This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.30 03:18:48.71 +71:20:47.5
134.23024 11.78424 galactic Cas Second-epoch detections are separated by 5.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543096144975925888 | 03:18:49.97 +71:20:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 18 48.71 +71 20 47.5 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543096144975925888,2461093.7619,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543096144975925888 20260222.2619 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:48.71 +71:20:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 15.03 +71 53 03.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543968229495046784,2461093.7619,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543968229495046784 20260222.2619 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:15.03 +71:53:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.37 03:21:57.40 +68:54:10.0
135.82214 9.88719 galactic Cas Second-epoch detections are separated by 3.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493106883181389184 | 03:21:58.78 +68:54:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 57.40 +68 54 10.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493106883181389184,2461093.7619,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493106883181389184 20260222.2619 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:57.40 +68:54:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 17 36.65 +73 18 06.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544340306804461568,2461093.7619,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544340306804461568 20260222.2619 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:36.65 +73:18:06.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.12 04:49:00.21 +70:52:23.8
140.02733 16.39940 galactic Cam Second-epoch detections are separated by 1.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 497412158397968896 | 04:49:01.58 +70:52:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 497412158397968896,2461093.7619,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 497412158397968896 20260222.2619 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:00.21 +70:52:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 49.95 +72 24 42.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:49.95 +72:24:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 27 23.44 +73 16 40.5 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:23.44 +73:16:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:24.68 +67:21:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482729658078182400,2461093.7619,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482729658078182400 20260222.2619 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:35.41 +65:43:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:37.97 +67:34:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:23.91 +65:47:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.46 04:59:11.91 +68:56:04.7
142.19505 15.96417 galactic Cam Second-epoch detections are separated by 3.4" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:11.91 +68:56:04.7 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.050 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:11.91 +68:56:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.30 04:39:00.14 +66:59:08.5
142.59407 13.27523 galactic Cam Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:00.14 +66:59:08.5 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:00.14 +66:59:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 490339824729520000,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490339824729520000 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:09:29.02 +66:45:48.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482360153451749888,2461093.7619,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482360153451749888 20260222.2619 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:39.91 +65:30:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:53.12 +66:22:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:24.68 +69:45:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.44 04:28:00.05 +70:46:05.3
138.97587 14.99934 galactic Cam Second-epoch detections are separated by 3.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:28:00.05 +70:46:05.3 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.050 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:00.05 +70:46:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:29.37 +70:10:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:36.61 +66:02:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:07.72 +65:11:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 25 43.28 +68 30 54.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493033044102975360,2461093.7619,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493033044102975360 20260222.2619 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:43.28 +68:30:54.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.38 04:57:14.40 +69:47:59.1
141.35648 16.32382 galactic Cam Second-epoch detections are separated by 1.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:14.40 +69:47:59.1 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.048 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:14.40 +69:47:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:52.39 +64:49:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.29 05:03:35.97 +68:40:11.3
142.65752 16.13989 galactic Cam Second-epoch detections are separated by 0.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:35.97 +68:40:11.3 (user input) | T | P | (position from user input) J-Ks=0.700+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:35.97 +68:40:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:05.38 +67:07:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.24 04:57:18.04 +73:03:08.3
138.57057 18.19518 galactic Cam Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:18.04 +73:03:08.3 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:18.04 +73:03:08.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 46.63 +71 53 16.4 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543956822062080384,2461093.7619,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543956822062080384 20260222.2619 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:46.63 +71:53:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 18 15.86 +71 31 05.7 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:15.86 +71:31:05.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.04 04:34:49.11 +66:05:18.4
143.01583 12.37561 galactic Cam Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:34:49.11 +66:05:18.4 (user input) | T | P | (position from user input) J-Ks=0.776+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:49.11 +66:05:18.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:59.86 +72:53:40.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:15.39 +68:25:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.21 04:24:10.30 +70:35:42.2
138.88889 14.64838 galactic Cam Second-epoch detections are separated by 0.9" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:10.30 +70:35:42.2 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:10.30 +70:35:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.06 03:23:44.73 +69:23:58.9
135.67660 10.38892 galactic Cas Second-epoch detections are separated by 5.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J050.9625+69.3975 | 03:23:44.73 +69:23:58.9 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 44.73 +69 23 58.9 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J050.9625+69.3975,2461093.7619,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J050.9625+69.3975 20260222.2619 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:44.73 +69:23:58.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 48.96 +71 16 02.0 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:48.96 +71:16:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:27.76 +67:16:28.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 35.25 +73 42 58.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:35.25 +73:42:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:53.77 +67:52:43.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 19 56.56 +70 59 48.9 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:56.56 +70:59:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.04 06:09:53.99 +68:10:40.9
146.04283 21.32614 galactic Cam Second-epoch detections are separated by 2.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:09:53.99 +68:10:40.9 (user input) | T | P | (position from user input) J-Ks=0.240+/-0.038 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:53.99 +68:10:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483457259898155136,2461093.7619,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483457259898155136 20260222.2619 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:37.36 +66:51:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 12.84 +72 04 33.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:12.84 +72:04:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 24 07.24 +70 13 44.0 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:07.24 +70:13:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 53.48 +70 34 05.8 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:53.48 +70:34:05.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:34.46 +67:15:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:04.83 +64:57:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 17 00.40 +70 50 19.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:00.40 +70:50:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 19 58.99 +69 16 23.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541165986673967616,2461093.7619,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541165986673967616 20260222.2619 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:58.99 +69:16:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 18 33.74 +71 46 41.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:33.74 +71:46:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496117827053125504,2461093.7619,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496117827053125504 20260222.2619 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:12.36 +68:55:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 25 46.72 +69 49 37.8 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:46.72 +69:49:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 26 46.00 +68 32 03.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:46.00 +68:32:03.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.71 03:09:36.37 +72:28:22.0
132.99961 12.35904 galactic Cas Second-epoch detections are separated by 6.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544151396962993024 | 03:09:34.13 +72:28:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 09 36.37 +72 28 22.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544151396962993024,2461093.7619,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544151396962993024 20260222.2619 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:36.37 +72:28:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 18.89 +69 58 47.0 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:18.89 +69:58:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 57.37 +71 26 46.7 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543181254047737984,2461093.7619,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543181254047737984 20260222.2619 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:57.37 +71:26:46.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 42.86 +72 17 50.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:42.86 +72:17:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.74 03:14:43.69 +73:15:53.3
132.90150 13.23102 galactic Cas Second-epoch detections are separated by 1.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544342127870595968 | 03:14:45.28 +73:15:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 14 43.69 +73 15 53.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544342127870595968,2461093.7619,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544342127870595968 20260222.2619 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:43.69 +73:15:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 24 26.83 +70 50 47.3 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:26.83 +70:50:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.59 03:18:14.36 +70:37:20.7
134.59197 11.15112 galactic Cas Second-epoch detections are separated by 2.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 542990832375500928 | 03:18:13.24 +70:37:18.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 18 14.36 +70 37 20.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 542990832375500928,2461093.7619,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 542990832375500928 20260222.2619 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:14.36 +70:37:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.66 04:32:07.34 +69:05:37.2
140.51523 14.15718 galactic Cam Second-epoch detections are separated by 0.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:32:07.34 +69:05:37.2 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:07.34 +69:05:37.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.62 03:24:25.53 +69:38:10.4
135.59221 10.61826 galactic Cas Second-epoch detections are separated by 4.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 542701381645520256 | 03:24:26.75 +69:38:13.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 24 25.53 +69 38 10.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 542701381645520256,2461093.7619,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 542701381645520256 20260222.2619 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:25.53 +69:38:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502345941947700608,2461093.7619,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502345941947700608 20260222.2619 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:07.22 +73:47:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.58 03:33:08.32 +67:23:34.8
137.56012 9.23641 galactic Cam Second-epoch detections are separated by 2.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 491977409860033152 | 03:33:09.56 +67:23:40.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 491977409860033152,2461093.7619,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 491977409860033152 20260222.2619 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:08.32 +67:23:34.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 26 32.55 +71 04 43.6 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:32.55 +71:04:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.53 03:19:31.94 +72:10:47.9
133.81213 12.51275 galactic Cas Second-epoch detections are separated by 1.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544023411234817408 | 03:19:29.70 +72:10:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 19 31.94 +72 10 47.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544023411234817408,2461093.7619,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544023411234817408 20260222.2619 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:31.94 +72:10:47.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.54 03:22:25.93 +73:51:49.3
133.03246 14.03059 galactic Cas Second-epoch detections are separated by 0.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544738368670911616 | 03:22:23.87 +73:51:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 22 25.93 +73 51 49.3 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544738368670911616,2461093.7619,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544738368670911616 20260222.2619 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:25.93 +73:51:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.29 03:34:37.84 +66:02:00.9
138.48711 8.22140 galactic Cam Second-epoch detections are separated by 7.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 491571518271211392 | 03:34:39.00 +66:02:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 491571518271211392,2461093.7619,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 491571518271211392 20260222.2619 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:37.84 +66:02:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.55 04:49:35.97 +70:19:02.2
140.52081 16.10420 galactic Cam Second-epoch detections are separated by 0.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:49:35.97 +70:19:02.2 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:35.97 +70:19:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.52 03:13:43.45 +71:55:12.5
133.56982 12.05266 galactic Cas Second-epoch detections are separated by 5.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543921770831597824 | 03:13:41.83 +71:55:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 43.45 +71 55 12.5 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543921770831597824,2461093.7619,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543921770831597824 20260222.2619 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:43.45 +71:55:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.61 04:40:25.93 +66:00:12.0
143.46104 12.75385 galactic Cam Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 483126989793606656 | 04:40:18.71 +66:00:13.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.728+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483126989793606656,2461093.7619,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483126989793606656 20260222.2619 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:25.93 +66:00:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 18 03.49 +72 49 34.1 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:03.49 +72:49:34.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.53 03:24:59.72 +68:07:51.3
136.49193 9.40025 galactic Cam Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493007270001094272 | 03:25:01.25 +68:07:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493007270001094272,2461093.7619,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493007270001094272 20260222.2619 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:59.72 +68:07:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.53 03:20:39.83 +69:14:05.7
135.53880 10.10116 galactic Cas Second-epoch detections are separated by 4.1" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 541164955881818496 | 03:20:41.39 +69:14:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 39.83 +69 14 05.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541164955881818496,2461093.7619,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541164955881818496 20260222.2619 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:39.83 +69:14:05.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.41 03:14:37.63 +71:48:15.1
133.69363 11.99170 galactic Cas Second-epoch detections are separated by 6.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543917304065614848 | 03:14:36.12 +71:48:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 14 37.63 +71 48 15.1 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543917304065614848,2461093.7619,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543917304065614848 20260222.2619 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:37.63 +71:48:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.35 03:42:11.71 +65:21:10.5
139.52864 8.14220 galactic Cam Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488521541735763584 | 03:42:11.77 +65:21:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488521541735763584,2461093.7619,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 488521541735763584 20260222.2619 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:11.71 +65:21:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.38 04:51:10.17 +67:30:35.6
142.92921 14.52119 galactic Cam Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:51:10.17 +67:30:35.6 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:10.17 +67:30:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.22 03:24:27.13 +69:27:01.7
135.70006 10.46573 galactic Cas Second-epoch detections are separated by 5.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J051.1185+69.4517 | 03:24:28.46 +69:27:06.4 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 24 27.13 +69 27 01.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J051.1185+69.4517,2461093.7619,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J051.1185+69.4517 20260222.2619 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:27.13 +69:27:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.24 03:13:47.53 +72:20:15.9
133.34793 12.40959 galactic Cas Second-epoch detections are separated by 3.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544137588646092544 | 03:13:45.60 +72:20:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 47.53 +72 20 15.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544137588646092544,2461093.7619,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544137588646092544 20260222.2619 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:47.53 +72:20:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.22 03:23:49.82 +68:53:43.6
135.96873 9.97461 galactic Cas Second-epoch detections are separated by 8.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493114987779200384 | 03:23:51.82 +68:53:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 49.82 +68 53 43.6 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493114987779200384,2461093.7619,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493114987779200384 20260222.2619 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:49.82 +68:53:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.16 03:22:15.19 +72:01:37.7
134.07710 12.50108 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543965068399262336 | 03:22:16.48 +72:01:41.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 22 15.19 +72 01 37.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543965068399262336,2461093.7619,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543965068399262336 20260222.2619 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:15.19 +72:01:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.94 03:20:52.60 +72:38:20.7
133.63939 12.95173 galactic Cas Second-epoch detections are separated by 7.3" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544074023129283968 | 03:20:50.89 +72:38:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 52.60 +72 38 20.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544074023129283968,2461093.7619,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544074023129283968 20260222.2619 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:52.60 +72:38:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.90 03:21:54.60 +72:12:50.2
133.94805 12.64153 galactic Cas Second-epoch detections are separated by 7.1" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543982145189001216 | 03:21:52.89 +72:12:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 54.60 +72 12 50.2 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543982145189001216,2461093.7619,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543982145189001216 20260222.2619 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:54.60 +72:12:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.29 03:20:49.92 +73:23:30.7
133.20751 13.57623 galactic Cas Second-epoch detections are separated by 2.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544297808105095808 | 03:20:51.25 +73:23:34.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 49.92 +73 23 30.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544297808105095808,2461093.7619,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544297808105095808 20260222.2619 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:49.92 +73:23:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.07 03:20:42.15 +69:26:29.3
135.42667 10.27580 galactic Cas Second-epoch detections are separated by 4.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 541193611903567232 | 03:20:43.27 +69:26:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 42.15 +69 26 29.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541193611903567232,2461093.7619,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541193611903567232 20260222.2619 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:42.15 +69:26:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.02 03:13:42.66 +71:26:02.0
133.83173 11.63946 galactic Cas Second-epoch detections are separated by 5.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 543840995382204032 | 03:13:44.05 +71:26:01.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 42.66 +71 26 02.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 543840995382204032,2461093.7619,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 543840995382204032 20260222.2619 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:42.66 +71:26:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 28.85 +72 15 44.2 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543983244700616064,2461093.7619,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543983244700616064 20260222.2619 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:28.85 +72:15:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 17 17.67 +71 01 34.9 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543063709382989696,2461093.7619,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543063709382989696 20260222.2619 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:17.67 +71:01:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.91 03:22:44.70 +72:13:06.0
133.99977 12.68076 galactic Cas Second-epoch detections are separated by 2.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543980495921757824 | 03:22:42.42 +72:13:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 22 44.70 +72 13 06.0 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543980495921757824,2461093.7619,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543980495921757824 20260222.2619 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:44.70 +72:13:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 25 49.03 +69 41 05.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 542691593416991232,2461093.7619,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 542691593416991232 20260222.2619 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:49.03 +69:41:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.93 05:52:27.95 +70:32:03.4
143.09217 20.75942 galactic Cam Second-epoch detections are separated by 1.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:52:27.95 +70:32:03.4 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:27.95 +70:32:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.79 03:25:46.42 +69:34:24.4
135.72694 10.63245 galactic Cas Second-epoch detections are separated by 2.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 542685786618852864 | 03:25:47.44 +69:34:28.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 25 46.42 +69 34 24.4 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 542685786618852864,2461093.7619,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 542685786618852864 20260222.2619 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:46.42 +69:34:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 20.24 +73 07 29.1 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544278768514463232,2461093.7619,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544278768514463232 20260222.2619 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:20.24 +73:07:29.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.73 03:13:23.56 +73:25:48.0
132.72786 13.31979 galactic Cas Second-epoch detections are separated by 3.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544356631977076096 | 03:13:24.92 +73:25:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 23.56 +73 25 48.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544356631977076096,2461093.7619,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544356631977076096 20260222.2619 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:23.56 +73:25:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.73 03:20:36.22 +69:40:29.2
135.28928 10.46617 galactic Cas Second-epoch detections are separated by 2.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 541251160167404032 | 03:20:37.74 +69:40:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 20 36.22 +69 40 29.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541251160167404032,2461093.7619,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541251160167404032 20260222.2619 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:36.22 +69:40:29.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.74 04:15:10.34 +68:05:26.0
140.18346 12.34278 galactic Cam Second-epoch detections are separated by 1.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 490571851744416384 | 04:15:07.57 +68:05:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 490571851744416384,2461093.7619,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490571851744416384 20260222.2619 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:10.34 +68:05:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.76 03:23:10.52 +72:10:59.6
134.04785 12.67009 galactic Cas Second-epoch detections are separated by 2.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543979499489346944 | 03:23:12.05 +72:11:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 10.52 +72 10 59.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543979499489346944,2461093.7619,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543979499489346944 20260222.2619 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:10.52 +72:10:59.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 16 15.61 +70 14 20.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541479862883756032,2461093.7619,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541479862883756032 20260222.2619 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:15.61 +70:14:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.78 06:03:45.46 +69:29:32.8
144.51322 21.26530 galactic Cam Second-epoch detections are separated by 2.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1107128013541125632 | 06:03:45.83 +69:29:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.280+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1107128013541125632,2461093.7619,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1107128013541125632 20260222.2619 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:45.46 +69:29:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.59 03:29:58.20 +73:49:29.5
133.49833 14.29964 galactic Cas Second-epoch detections are separated by 0.4" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544702634543178496 | 03:29:54.76 +73:49:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 29 58.20 +73 49 29.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544702634543178496,2461093.7619,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544702634543178496 20260222.2619 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:58.20 +73:49:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.41 03:25:16.25 +69:12:39.7
135.89752 10.30816 galactic Cas Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493137394627803136 | 03:25:15.15 +69:12:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 25 16.25 +69 12 39.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493137394627803136,2461093.7619,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493137394627803136 20260222.2619 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:16.25 +69:12:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.52 04:05:44.65 +69:16:48.3
138.70580 12.60112 galactic Cam Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493935979369184384 | 04:05:40.89 +69:16:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493935979369184384,2461093.7619,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493935979369184384 20260222.2619 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:44.65 +69:16:48.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.24 03:24:18.62 +72:38:27.2
133.85620 13.09660 galactic Cas Second-epoch detections are separated by 6.3" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544065879871265024 | 03:24:17.32 +72:38:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 24 18.62 +72 38 27.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544065879871265024,2461093.7619,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544065879871265024 20260222.2619 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:18.62 +72:38:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.21 03:19:09.10 +71:46:37.1
134.01297 12.15951 galactic Cas Second-epoch detections are separated by 7.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543873564118673664 | 03:19:10.75 +71:46:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 19 09.10 +71 46 37.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543873564118673664,2461093.7619,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543873564118673664 20260222.2619 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:09.10 +71:46:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.02 03:21:16.18 +72:46:17.9
133.58883 13.07822 galactic Cas Second-epoch detections are separated by 6.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 544077218582778368 | 03:21:14.48 +72:46:17.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 21 16.18 +72 46 17.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 544077218582778368,2461093.7619,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 544077218582778368 20260222.2619 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:16.18 +72:46:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.12 04:49:40.41 +66:03:58.7
144.01558 13.52382 galactic Cam Second-epoch detections are separated by 1.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 482433923811085696 | 04:49:39.22 +66:03:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.979+/-0.035 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482433923811085696,2461093.7619,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482433923811085696 20260222.2619 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:40.41 +66:03:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J033235.92+670747.8,2461093.7619,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J033235.92+670747.8 20260222.2619 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:34.88 +67:07:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 10.26 03:34:51.75 +66:55:44.1
137.97317 8.95891 galactic Cam Second-epoch detections are separated by 7.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 491904910812479104 | 03:34:52.68 +66:55:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 491904910812479104,2461093.7619,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 491904910812479104 20260222.2619 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:51.75 +66:55:44.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 10.11 03:23:09.53 +73:26:44.5
133.31814 13.71370 galactic Cas Second-epoch detections are separated by 7.0" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544674077304568064 | 03:23:08.12 +73:26:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1956PMcCO..13a....B AG+73 86
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 23 09.53 +73 26 44.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544674077304568064,2461093.7619,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544674077304568064 20260222.2619 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:09.53 +73:26:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 10.58 03:32:41.33 +65:47:02.6
138.47199 7.90312 galactic Cam Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 491562138062799616 | 03:32:42.50 +65:47:12.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 491562138062799616,2461093.7619,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 491562138062799616 20260222.2619 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:41.33 +65:47:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 10.85 03:28:50.03 +67:18:28.0
137.26750 8.92734 galactic Cam Second-epoch detections are separated by 3.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 492723497219854464 | 03:28:51.44 +67:18:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 492723497219854464,2461093.7619,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 492723497219854464 20260222.2619 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:50.03 +67:18:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 10.93 03:11:45.29 +71:39:17.0
133.57871 11.74599 galactic Cas Second-epoch detections are separated by 6.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543894115539708672 | 03:11:47.52 +71:39:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 11 45.29 +71 39 17.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543894115539708672,2461093.7619,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543894115539708672 20260222.2619 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:45.29 +71:39:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.14 03:36:03.85 +65:41:48.0
138.80731 8.03565 galactic Cam Second-epoch detections are separated by 0.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 491504963458109056 | 03:36:04.35 +65:41:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 491504963458109056,2461093.7619,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 491504963458109056 20260222.2619 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:03.85 +65:41:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.23 04:29:51.41 +65:59:09.4
142.75209 11.93084 galactic Cam Second-epoch detections are separated by 0.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 477356104234708480 | 04:29:53.21 +65:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 477356104234708480,2461093.7619,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477356104234708480 20260222.2619 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:51.41 +65:59:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.30 04:42:14.61 +69:04:10.8
141.13404 14.83370 galactic Cam Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:42:14.61 +69:04:10.8 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:14.61 +69:04:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.30 03:35:47.13 +64:54:42.0
139.25150 7.38502 galactic Cam Second-epoch detections are separated by 0.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488440143517235712 | 03:35:47.66 +64:54:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.197+/-0.149 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488440143517235712,2461093.7619,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 488440143517235712 20260222.2619 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:47.13 +64:54:42.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.74 03:09:56.56 +72:04:47.6
133.22979 12.03593 galactic Cas Second-epoch detections are separated by 6.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544104259699958784 | 03:09:58.65 +72:04:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 09 56.56 +72 04 47.6 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544104259699958784,2461093.7619,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544104259699958784 20260222.2619 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:56.56 +72:04:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.71 05:46:27.83 +68:07:42.4
145.19998 19.29444 galactic Cam Second-epoch detections are separated by 0.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 481671859173539200 | 05:46:29.06 +68:08:10.9 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE J-Ks=0.373+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 481671859173539200,2461093.7619,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 481671859173539200 20260222.2619 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:27.83 +68:07:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.71 03:37:57.98 +64:58:21.5
139.40253 7.57107 galactic Cam Second-epoch detections are separated by 1.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488417294290142080 | 03:37:58.40 +64:58:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488417294290142080,2461093.7619,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 488417294290142080 20260222.2619 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:57.98 +64:58:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.74 04:42:28.43 +68:14:34.9
141.81182 14.33021 galactic Cam Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495662320001516416 | 04:42:27.40 +68:15:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.665+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495662320001516416,2461093.7619,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495662320001516416 20260222.2619 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:28.43 +68:14:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.79 03:14:32.41 +71:22:49.7
133.91785 11.62918 galactic Cas Second-epoch detections are separated by 1.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543836906575381888 | 03:14:28.01 +71:22:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 14 32.41 +71 22 49.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543836906575381888,2461093.7619,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543836906575381888 20260222.2619 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:32.41 +71:22:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0418017+711356,2461093.7619,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0418017+711356 20260222.2619 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:01.21 +71:13:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.88 03:08:43.76 +72:37:13.7
132.86400 12.45174 galactic Cas Second-epoch detections are separated by 6.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544200737547278464 | 03:08:45.08 +72:37:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 08 43.76 +72 37 13.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544200737547278464,2461093.7619,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544200737547278464 20260222.2619 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:43.76 +72:37:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 11.89 03:26:52.29 +67:44:42.9
136.85946 9.18067 galactic Cam Second-epoch detections are separated by 4.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 492795961908091392 | 03:26:53.88 +67:44:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 492795961908091392,2461093.7619,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 492795961908091392 20260222.2619 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:52.29 +67:44:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.05 05:32:38.92 +71:28:26.7
141.45778 19.69686 galactic Cam Second-epoch detections are separated by 0.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 498286407580396416 | 05:32:44.24 +71:28:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.634+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 498286407580396416,2461093.7619,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 498286407580396416 20260222.2619 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:38.92 +71:28:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.13 03:09:13.36 +73:06:14.4
132.64061 12.88489 galactic Cas Second-epoch detections are separated by 6.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544324849219137280 | 03:09:15.04 +73:06:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 09 13.36 +73 06 14.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544324849219137280,2461093.7619,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544324849219137280 20260222.2619 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:13.36 +73:06:14.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.13 03:13:18.84 +71:39:25.6
133.68409 11.81243 galactic Cas Second-epoch detections are separated by 3.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543892358895565184 | 03:13:20.96 +71:39:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 18.84 +71 39 25.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543892358895565184,2461093.7619,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543892358895565184 20260222.2619 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:18.84 +71:39:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.19 04:29:19.30 +69:15:32.7
140.21755 14.07988 galactic Cam Second-epoch detections are separated by 2.4" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:29:19.30 +69:15:32.7 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:19.30 +69:15:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.21 04:10:08.78 +68:21:09.3
139.65522 12.20298 galactic Cam Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:10:08.78 +68:21:09.3 (user input) | T | P | (position from user input) J-Ks=0.231+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:08.78 +68:21:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.23 03:06:41.53 +73:20:49.8
132.35190 13.00017 galactic Cas Second-epoch detections are separated by 7.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 547334418703037440 | 03:06:42.51 +73:20:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 06 41.53 +73 20 49.8 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 547334418703037440,2461093.7619,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 547334418703037440 20260222.2619 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:06:41.53 +73:20:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.35 03:15:59.00 +70:17:15.3
134.61354 10.76737 galactic Cas Second-epoch detections are separated by 1.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 541483127058887680 | 03:16:00.52 +70:17:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 15 59.00 +70 17 15.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541483127058887680,2461093.7619,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541483127058887680 20260222.2619 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:59.00 +70:17:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:41.43 +70:26:56.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.55 04:50:22.61 +72:53:49.7
138.39482 17.69224 galactic Cam Second-epoch detections are separated by 1.4" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:50:22.61 +72:53:49.7 (user input) | T | P | (position from user input) J-Ks=0.853+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:22.61 +72:53:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.48 06:00:09.66 +68:03:11.5
145.81817 20.43453 galactic Cam Second-epoch detections are separated by 5.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1105448410749520768 | 06:00:10.44 +68:03:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1105448410749520768,2461093.7619,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1105448410749520768 20260222.2619 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:09.66 +68:03:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.48 04:45:55.60 +68:04:56.1
142.14853 14.48050 galactic Cam Second-epoch detections are separated by 7.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495600369393497600 | 04:45:51.14 +68:05:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495600369393497600,2461093.7619,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495600369393497600 20260222.2619 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:55.60 +68:04:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:16.55 +72:56:16.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.45 03:15:43.29 +70:14:29.2
134.61958 10.71656 galactic Cas Second-epoch detections are separated by 2.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 541477178525619456 | 03:15:44.26 +70:14:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 15 43.29 +70 14 29.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541477178525619456,2461093.7619,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541477178525619456 20260222.2619 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:43.29 +70:14:29.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.54 03:38:02.44 +65:09:10.1
139.30041 7.72033 galactic Cam Second-epoch detections are separated by 3.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488468486001497216 | 03:38:02.97 +65:09:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488468486001497216,2461093.7619,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 488468486001497216 20260222.2619 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:02.44 +65:09:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.55 03:16:53.37 +73:32:41.2
132.88003 13.55002 galactic Cas Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544352573231049984 | 03:16:55.62 +73:32:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 16 53.37 +73 32 41.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544352573231049984,2461093.7619,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544352573231049984 20260222.2619 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:53.37 +73:32:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 12 39.36 +73 32 41.3 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544361407980700160,2461093.7619,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544361407980700160 20260222.2619 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:39.36 +73:32:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:07.66 +66:28:22.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 15 09.25 +72 27 59.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J031510.36+722803.7,2461093.7619,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J031510.36+722803.7 20260222.2619 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:09.25 +72:27:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.46 03:11:13.68 +71:48:52.0
133.45761 11.86072 galactic Cas Second-epoch detections are separated by 5.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543909779282889728 | 03:11:15.93 +71:48:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 11 13.68 +71 48 52.0 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543909779282889728,2461093.7619,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543909779282889728 20260222.2619 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:13.68 +71:48:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.64 05:30:38.77 +74:24:25.9
138.59748 20.89185 galactic Cam Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502746267259163264 | 05:30:33.34 +74:23:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.370+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502746267259163264,2461093.7619,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502746267259163264 20260222.2619 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:38.77 +74:24:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.57 03:13:02.10 +71:17:23.4
133.86242 11.48858 galactic Cas Second-epoch detections are separated by 5.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543830786244422784 | 03:13:04.26 +71:17:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 13 02.10 +71 17 23.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543830786244422784,2461093.7619,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543830786244422784 20260222.2619 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:02.10 +71:17:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.70 04:55:33.28 +66:54:53.6
143.68403 14.50386 galactic Cam Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:33.28 +66:54:53.6 (user input) | T | P | (position from user input) J-Ks=0.664+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:33.28 +66:54:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.72 04:46:15.03 +66:27:35.9
143.47833 13.49674 galactic Cam Second-epoch detections are separated by 1.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 483234810651741952 | 04:46:12.01 +66:27:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.932+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483234810651741952,2461093.7619,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483234810651741952 20260222.2619 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:15.03 +66:27:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:10.74 +65:24:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.68 04:56:31.70 +72:51:33.2
138.70363 18.03869 galactic Cam Second-epoch detections are separated by 2.3" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:31.70 +72:51:33.2 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.040 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:31.70 +72:51:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:29.66 +69:08:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:04.35 +65:03:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.78 03:12:37.20 +71:01:07.3
133.97858 11.24024 galactic Cas Second-epoch detections are separated by 2.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 542313116600733568 | 03:12:40.14 +71:01:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 12 37.20 +71 01 07.3 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 542313116600733568,2461093.7619,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 542313116600733568 20260222.2619 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:37.20 +71:01:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 12 17.32 +71 03 39.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:17.32 +71:03:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:55.95 +69:09:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J033506.8+653200,2461093.7619,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J033506.8+653200 20260222.2619 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:06.48 +65:31:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:50.35 +66:06:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.95 05:03:33.67 +65:44:41.9
145.14948 14.47312 galactic Cam Second-epoch detections are separated by 1.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:33.67 +65:44:41.9 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:33.67 +65:44:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.89 04:38:34.80 +65:24:54.1
143.79607 12.22907 galactic Cam Second-epoch detections are separated by 2.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:38:34.80 +65:24:54.1 (user input) | T | P | (position from user input) J-Ks=0.756+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:34.80 +65:24:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.81 03:08:56.28 +72:42:54.3
132.82781 12.54087 galactic Cas Second-epoch detections are separated by 6.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544210049036370432 | 03:08:57.91 +72:43:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 08 56.28 +72 42 54.3 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544210049036370432,2461093.7619,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544210049036370432 20260222.2619 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:56.28 +72:42:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 14 52.33 +70 17 28.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:52.33 +70:17:28.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.99 04:20:01.18 +68:13:23.8
140.40981 12.75761 galactic Cam Second-epoch detections are separated by 3.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:20:01.18 +68:13:23.8 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.046 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:01.18 +68:13:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496326425025087744,2461093.7619,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496326425025087744 20260222.2619 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:41.80 +69:27:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 15 35.81 +72 24 24.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544044095797285888,2461093.7619,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544044095797285888 20260222.2619 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:35.81 +72:24:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.93 03:16:22.28 +73:26:00.9
132.91016 13.43661 galactic Cas Second-epoch detections are separated by 7.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544345082808089856 | 03:16:24.23 +73:26:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 16 22.28 +73 26 00.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544345082808089856,2461093.7619,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544345082808089856 20260222.2619 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:22.28 +73:26:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:15.36 +71:09:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.01 05:41:41.51 +70:56:51.3
142.30204 20.11775 galactic Cam Second-epoch detections are separated by 3.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:41:41.51 +70:56:51.3 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:41.51 +70:56:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:27.85 +65:16:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.18 04:41:43.29 +68:50:32.3
141.28631 14.65425 galactic Cam Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:41:43.29 +68:50:32.3 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:43.29 +68:50:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:29.01 +74:16:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:36.69 +68:12:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.05 05:01:54.70 +71:44:41.0
139.91289 17.74703 galactic Cam Second-epoch detections are separated by 1.1" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 497558393443830656 | 05:01:57.82 +71:45:16.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.454+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 497558393443830656,2461093.7619,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 497558393443830656 20260222.2619 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:54.70 +71:44:41.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.99 05:15:55.39 +73:40:00.6
138.77785 19.64954 galactic Cam Second-epoch detections are separated by 0.8" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:15:55.39 +73:40:00.6 (user input) | T | P | (position from user input) J-Ks=0.726+/-0.027 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:55.39 +73:40:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502494650896497920,2461093.7619,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502494650896497920 20260222.2619 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:27.05 +73:55:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.99 04:11:33.52 +65:34:23.1
141.72259 10.29674 galactic Cam Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:11:33.52 +65:34:23.1 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.027 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:33.52 +65:34:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.12 05:18:29.74 +68:23:54.5
143.66472 17.13938 galactic Cam Second-epoch detections are separated by 1.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | KELT KC18C012925 | 05:18:31.30 +68:24:38.8 (Gaia DR3) | EA (local) | 2458029.66000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.039 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KELT KC18C012925,2461093.7619,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KELT KC18C012925 20260222.2619 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:29.74 +68:23:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 17 52.20 +69 28 34.6 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 541221649449776384,2461093.7619,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541221649449776384 20260222.2619 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:52.20 +69:28:34.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:44.09 +73:30:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.16 04:52:20.32 +66:13:58.9
144.04876 13.83900 galactic Cam Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 482442135787179520 | 04:52:26.68 +66:14:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.151+/-0.049 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482442135787179520,2461093.7619,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482442135787179520 20260222.2619 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:20.32 +66:13:58.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.26 04:41:09.29 +67:50:55.8
142.04651 13.98553 galactic Cam Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495571163616051456 | 04:41:05.49 +67:51:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.409+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495571163616051456,2461093.7619,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495571163616051456 20260222.2619 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:09.29 +67:50:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.20 05:13:37.00 +68:17:16.8
143.51576 16.69834 galactic Cam Second-epoch detections are separated by 1.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 485283273832857344 | 05:13:34.08 +68:16:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.631+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 485283273832857344,2461093.7619,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485283273832857344 20260222.2619 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:37.00 +68:17:16.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:14.70 +71:13:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483565458713772672,2461093.7619,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483565458713772672 20260222.2619 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:38.69 +67:36:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2619* 03 12 41.44 +71 22 37.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:41.44 +71:22:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.14 04:43:33.40 +68:31:39.8
141.64756 14.58652 galactic Cam Second-epoch detections are separated by 1.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:43:33.40 +68:31:39.8 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:43:33.40 +68:31:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.27 04:24:11.86 +67:34:11.7
141.17285 12.59291 galactic Cam Second-epoch detections are separated by 2.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:11.86 +67:34:11.7 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:11.86 +67:34:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.29 04:54:16.80 +65:21:24.4
144.89104 13.46819 galactic Cam Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:16.80 +65:21:24.4 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.039 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:16.80 +65:21:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.24 05:07:59.96 +65:47:23.5
145.37800 14.87378 galactic Cam Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 479590827261511936 | 05:08:04.72 +65:47:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 479590827261511936,2461093.7619,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 479590827261511936 20260222.2619 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:59.96 +65:47:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.24 05:44:28.44 +64:32:51.6
148.50352 17.55105 galactic Cam Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 287796069060255744 | 05:44:28.47 +64:32:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 287796069060255744,2461093.7619,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287796069060255744 20260222.2619 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:28.44 +64:32:51.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.43 05:14:42.86 +74:54:33.0
137.59156 20.20296 galactic Cam Second-epoch detections are separated by 0.8" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:14:42.86 +74:54:33.0 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:42.86 +74:54:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.41 05:02:51.25 +66:09:46.2
144.75323 14.65398 galactic Cam Second-epoch detections are separated by 2.6" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 482580841752568448 | 05:02:51.79 +66:10:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.660+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482580841752568448,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482580841752568448 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:51.25 +66:09:46.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:00.75 +64:59:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:08.07 +67:40:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.49 06:15:00.15 +70:38:30.3
143.68800 22.55075 galactic Cam Second-epoch detections are separated by 1.5" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:15:00.15 +70:38:30.3 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.045 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:00.15 +70:38:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.39 05:01:00.33 +67:24:59.2
143.58350 15.22617 galactic Cam Second-epoch detections are separated by 0.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 483639744469264896 | 05:00:53.13 +67:24:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.472+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483639744469264896,2461093.7619,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483639744469264896 20260222.2619 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:00.33 +67:24:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.46 05:54:40.37 +71:02:25.3
142.66711 21.12203 galactic Cam Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:54:40.37 +71:02:25.3 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:40.37 +71:02:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:14.73 +73:37:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.39 05:29:51.59 +72:20:59.2
140.52522 19.90617 galactic Cam Second-epoch detections are separated by 0.7" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:29:51.59 +72:20:59.2 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:51.59 +72:20:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.35 04:10:47.07 +70:07:30.0
138.42994 13.51362 galactic Cam Second-epoch detections are separated by 4.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 494177906286853120 | 04:10:47.67 +70:06:56.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 494177906286853120,2461093.7619,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494177906286853120 20260222.2619 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:47.07 +70:07:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.41 05:38:34.10 +72:33:43.1
140.63439 20.58820 galactic Cam Second-epoch detections are separated by 2.8" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:38:34.10 +72:33:43.1 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.040 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:34.10 +72:33:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.36 05:08:36.53 +67:53:18.6
143.60159 16.08918 galactic Cam Second-epoch detections are separated by 1.4" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:36.53 +67:53:18.6 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.057 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:36.53 +67:53:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.44 04:58:07.28 +67:47:56.5
143.09541 15.22430 galactic Cam Second-epoch detections are separated by 1.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:07.28 +67:47:56.5 (user input) | T | P | (position from user input) J-Ks=0.667+/-0.040 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:07.28 +67:47:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:46.66 +71:04:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.57 04:37:51.24 +68:09:14.6
141.60105 13.94275 galactic Cam Second-epoch detections are separated by 5.4" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:51.24 +68:09:14.6 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:51.24 +68:09:14.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.52 04:18:30.24 +65:45:02.5
142.11361 10.92591 galactic Cam Second-epoch detections are separated by 2.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:18:30.24 +65:45:02.5 (user input) | T | P | (position from user input) J-Ks=0.771+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:30.24 +65:45:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:09.12 +65:02:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.51 05:34:04.06 +68:50:00.1
143.99857 18.58926 galactic Cam Second-epoch detections are separated by 1.5" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:04.06 +68:50:00.1 (user input) | T | P | (position from user input) J-Ks=0.284+/-0.049 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:04.06 +68:50:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.39 05:46:03.79 +71:54:41.3
141.52150 20.83571 galactic Cam Second-epoch detections are separated by 1.8" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:46:03.79 +71:54:41.3 (user input) | T | P | (position from user input) J-Ks=0.536+/-0.048 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:03.79 +71:54:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.49 05:18:32.04 +70:53:23.7
141.41925 18.41827 galactic Cam Second-epoch detections are separated by 1.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:18:32.04 +70:53:23.7 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.046 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:32.04 +70:53:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.51 04:58:39.37 +66:34:13.5
144.15795 14.54776 galactic Cam Second-epoch detections are separated by 0.9" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:39.37 +66:34:13.5 (user input) | T | P | (position from user input) J-Ks=0.788+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:39.37 +66:34:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.53 05:33:07.50 +73:20:44.2
139.69533 20.57198 galactic Cam Second-epoch detections are separated by 1.1" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:33:07.50 +73:20:44.2 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:07.50 +73:20:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.56 04:53:10.49 +66:33:43.0
143.83077 14.10441 galactic Cam Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:10.49 +66:33:43.0 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.049 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:10.49 +66:33:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.59 05:35:59.02 +70:13:11.9
142.77546 19.37222 galactic Cam Second-epoch detections are separated by 2.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:59.02 +70:13:11.9 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:59.02 +70:13:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:01.40 +66:58:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.42 05:07:54.88 +70:14:26.2
141.51143 17.32563 galactic Cam Second-epoch detections are separated by 0.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 497742286763586816 | 05:08:02.36 +70:14:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.482+/-0.048 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 497742286763586816,2461093.7619,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 497742286763586816 20260222.2619 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:54.88 +70:14:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.36 04:39:44.78 +68:25:39.5
141.49987 14.25233 galactic Cam Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:44.78 +68:25:39.5 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:44.78 +68:25:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 485855088599053440,2461093.7619,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485855088599053440 20260222.2619 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:48.94 +69:57:50.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.55 04:15:10.29 +69:56:54.5
138.83111 13.65259 galactic Cam Second-epoch detections are separated by 1.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:15:10.29 +69:56:54.5 (user input) | T | P | (position from user input) J-Ks=0.740+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:10.29 +69:56:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.71 04:59:06.11 +65:22:21.5
145.18576 13.88139 galactic Cam Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:06.11 +65:22:21.5 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:06.11 +65:22:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.59 05:46:20.74 +71:28:22.1
141.95968 20.67748 galactic Cam Second-epoch detections are separated by 2.5" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:46:20.74 +71:28:22.1 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:20.74 +71:28:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.43 05:24:14.41 +73:27:32.5
139.27663 20.06088 galactic Cam Second-epoch detections are separated by 1.6" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:24:14.41 +73:27:32.5 (user input) | T | P | (position from user input) J-Ks=0.266+/-0.049 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:14.41 +73:27:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.60 05:23:27.76 +69:02:17.2
143.32701 17.85245 galactic Cam Second-epoch detections are separated by 0.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:23:27.76 +69:02:17.2 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.044 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:27.76 +69:02:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.29 04:51:08.18 +69:25:23.5
141.34637 15.67246 galactic Cam Second-epoch detections are separated by 3.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496296841290259328 | 04:51:10.13 +69:26:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496296841290259328,2461093.7619,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496296841290259328 20260222.2619 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:08.18 +69:25:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.54 05:03:50.20 +67:50:15.1
143.38451 15.68780 galactic Cam Second-epoch detections are separated by 4.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:50.20 +67:50:15.1 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.061 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:50.20 +67:50:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.59 05:54:24.79 +67:33:38.3
146.07667 19.74298 galactic Cam Second-epoch detections are separated by 2.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:54:24.79 +67:33:38.3 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:24.79 +67:33:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.49 05:29:37.95 +70:26:14.1
142.31044 18.99808 galactic Cam Second-epoch detections are separated by 1.6" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 485800868927773952 | 05:29:37.95 +70:26:14.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.454+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 485800868927773952,2461093.7619,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 485800868927773952 20260222.2619 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:37.95 +70:26:14.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.45 04:26:02.56 +66:20:55.3
142.21272 11.89202 galactic Cam Second-epoch detections are separated by 2.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:26:02.56 +66:20:55.3 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:02.56 +66:20:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.58 05:30:09.22 +72:28:21.0
140.42021 19.98239 galactic Cam Second-epoch detections are separated by 1.2" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:30:09.22 +72:28:21.0 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:09.22 +72:28:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 05:26:36.97 +71:07:51.0
141.54000 19.10906 galactic Cam Second-epoch detections are separated by 0.8" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:26:36.97 +71:07:51.0 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.054 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:36.97 +71:07:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.46 04:24:34.49 +67:41:11.5
141.11063 12.69874 galactic Cam Second-epoch detections are separated by 2.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:34.49 +67:41:11.5 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.075 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:34.49 +67:41:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.63 04:15:07.08 +69:52:49.4
138.87759 13.60144 galactic Cam Second-epoch detections are separated by 1.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:15:07.08 +69:52:49.4 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.042 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:07.08 +69:52:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.74 05:40:11.87 +69:35:20.3
143.54528 19.41571 galactic Cam Second-epoch detections are separated by 3.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:11.87 +69:35:20.3 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:11.87 +69:35:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045246.90+674923.1,2461093.7619,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045246.90+674923.1 20260222.2619 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:47.11 +67:49:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.68 04:56:09.41 +64:58:46.4
145.32284 13.39941 galactic Cam Second-epoch detections are separated by 0.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:09.41 +64:58:46.4 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:09.41 +64:58:46.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.41 04:44:18.83 +65:11:40.3
144.36187 12.54824 galactic Cam Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:44:18.83 +65:11:40.3 (user input) | T | P | (position from user input) J-Ks=0.805+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:18.83 +65:11:40.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.64 05:20:36.16 +66:22:27.7
145.58212 16.26455 galactic Cam Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:20:36.16 +66:22:27.7 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:36.16 +66:22:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.43 04:56:10.62 +65:17:00.3
145.07356 13.58265 galactic Cam Second-epoch detections are separated by 3.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:10.62 +65:17:00.3 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.044 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:10.62 +65:17:00.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.52 06:07:10.88 +71:30:10.1
142.58655 22.22477 galactic Cam Second-epoch detections are separated by 1.0" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:07:10.88 +71:30:10.1 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:10.88 +71:30:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.56 04:32:38.51 +65:48:33.5
143.08052 12.02475 galactic Cam Second-epoch detections are separated by 1.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:32:38.51 +65:48:33.5 (user input) | T | P | (position from user input) J-Ks=0.804+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:38.51 +65:48:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.54 05:14:49.52 +68:54:52.3
143.02170 17.12408 galactic Cam Second-epoch detections are separated by 1.0" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:14:49.52 +68:54:52.3 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.062 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:49.52 +68:54:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.57 05:25:27.29 +68:03:13.0
144.31866 17.52107 galactic Cam Second-epoch detections are separated by 1.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:25:27.29 +68:03:13.0 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:27.29 +68:03:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.65 05:05:57.61 +67:42:12.8
143.61701 15.77837 galactic Cam Second-epoch detections are separated by 1.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 483732137803597184 | 05:05:57.61 +67:42:12.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.409+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 483732137803597184,2461093.7619,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 483732137803597184 20260222.2619 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:57.61 +67:42:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.51 05:27:08.09 +72:06:04.5
140.65563 19.60625 galactic Cam Second-epoch detections are separated by 1.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:27:08.09 +72:06:04.5 (user input) | T | P | (position from user input) J-Ks=0.665+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:08.09 +72:06:04.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 05:10:25.35 +72:12:14.9
139.88349 18.54931 galactic Cam Second-epoch detections are separated by 1.4" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:10:25.35 +72:12:14.9 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.049 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:25.35 +72:12:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:40.13 +64:59:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.41 04:12:20.14 +68:01:10.0
140.04191 12.10580 galactic Cam Second-epoch detections are separated by 2.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:12:20.14 +68:01:10.0 (user input) | T | P | (position from user input) J-Ks=0.630+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:20.14 +68:01:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.62 04:57:11.50 +68:24:56.5
142.52387 15.51426 galactic Cam Second-epoch detections are separated by 0.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:11.50 +68:24:56.5 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.057 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:11.50 +68:24:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.72 04:38:02.78 +65:40:20.5
143.55888 12.35381 galactic Cam Second-epoch detections are separated by 4.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:38:02.78 +65:40:20.5 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.043 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:02.78 +65:40:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.56 04:36:00.62 +66:19:30.3
142.91330 12.62143 galactic Cam Second-epoch detections are separated by 1.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:36:00.62 +66:19:30.3 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:36:00.62 +66:19:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.73 04:39:28.54 +68:08:45.8
141.70706 14.05344 galactic Cam Second-epoch detections are separated by 0.3" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:28.54 +68:08:45.8 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:28.54 +68:08:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.59 05:37:58.51 +72:33:47.4
140.61280 20.54861 galactic Cam Second-epoch detections are separated by 0.8" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:37:58.51 +72:33:47.4 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:58.51 +72:33:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 484450359415942656,2461093.7619,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 484450359415942656 20260222.2619 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:43.20 +67:43:19.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.68 05:15:42.78 +70:06:35.3
141.99657 17.81586 galactic Cam Second-epoch detections are separated by 2.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:15:42.78 +70:06:35.3 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.069 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:42.78 +70:06:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 05:49:03.77 +70:50:50.0
142.66590 20.62507 galactic Cam Second-epoch detections are separated by 3.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:49:03.77 +70:50:50.0 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.055 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:03.77 +70:50:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:31.96 +73:04:27.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.70 05:32:07.06 +69:18:10.7
143.47447 18.65398 galactic Cam Second-epoch detections are separated by 3.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:32:07.06 +69:18:10.7 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:07.06 +69:18:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:51.56 +66:17:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:55.30 +66:34:55.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.54 06:02:29.94 +73:26:04.8
140.48996 22.53736 galactic Cam Second-epoch detections are separated by 0.9" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:02:29.94 +73:26:04.8 (user input) | T | P | (position from user input) J-Ks=0.494+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:29.94 +73:26:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:57.75 +66:13:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.75 05:40:39.98 +72:33:22.0
140.71159 20.72795 galactic Cam Second-epoch detections are separated by 0.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:40:39.98 +72:33:22.0 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.048 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:39.98 +72:33:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.63 05:19:24.42 +67:05:13.2
144.88320 16.53335 galactic Cam Second-epoch detections are separated by 4.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:24.42 +67:05:13.2 (user input) | T | P | (position from user input) J-Ks=0.695+/-0.042 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:24.42 +67:05:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.47 04:53:12.16 +70:21:09.7
140.67949 16.36864 galactic Cam Second-epoch detections are separated by 1.7" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:12.16 +70:21:09.7 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.039 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:12.16 +70:21:09.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.57 05:25:52.22 +71:45:50.9
140.92088 19.35984 galactic Cam Second-epoch detections are separated by 2.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:25:52.22 +71:45:50.9 (user input) | T | P | (position from user input) J-Ks=0.546+/-0.047 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:52.22 +71:45:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.74 05:12:16.01 +71:06:23.0
140.94648 18.09345 galactic Cam Second-epoch detections are separated by 2.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:12:16.01 +71:06:23.0 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.064 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:16.01 +71:06:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.64 04:04:56.61 +69:20:11.2
138.61342 12.59401 galactic Cam Second-epoch detections are separated by 2.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:04:56.61 +69:20:11.2 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:04:56.61 +69:20:11.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.74 04:32:57.88 +67:16:23.9
141.97765 13.01733 galactic Cam Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:32:57.88 +67:16:23.9 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:57.88 +67:16:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489917887142564224,2461093.7619,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489917887142564224 20260222.2619 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:25.46 +66:01:48.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483302125678761984,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483302125678761984 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:48.44 +65:59:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.63 04:42:27.97 +68:36:51.8
141.51327 14.56328 galactic Cam Second-epoch detections are separated by 2.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:42:27.97 +68:36:51.8 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:27.97 +68:36:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 484173385565411584,2461093.7619,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 484173385565411584 20260222.2619 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:23.77 +66:54:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.49 05:03:25.11 +68:43:25.9
142.60140 16.15681 galactic Cam Second-epoch detections are separated by 1.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:25.11 +68:43:25.9 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:25.11 +68:43:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:42.61 +68:55:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.64 04:29:28.68 +69:15:10.9
140.23170 14.08619 galactic Cam Second-epoch detections are separated by 3.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:29:28.68 +69:15:10.9 (user input) | T | P | (position from user input) J-Ks=0.732+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:28.68 +69:15:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.71 05:58:11.41 +73:30:51.0
140.29510 22.27707 galactic Cam Second-epoch detections are separated by 1.7" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:58:11.41 +73:30:51.0 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:11.41 +73:30:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.66 05:28:51.53 +70:26:47.6
142.26941 18.94542 galactic Cam Second-epoch detections are separated by 3.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:28:51.53 +70:26:47.6 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:51.53 +70:26:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.56 05:08:12.10 +70:39:45.2
141.15373 17.57498 galactic Cam Second-epoch detections are separated by 2.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:12.10 +70:39:45.2 (user input) | T | P | (position from user input) J-Ks=0.235+/-0.076 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:12.10 +70:39:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.53 05:07:06.59 +65:02:37.5
145.96187 14.37772 galactic Cam Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:06.59 +65:02:37.5 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:06.59 +65:02:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.59 05:17:51.78 +68:38:01.5
143.42266 17.21166 galactic Cam Second-epoch detections are separated by 1.4" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:51.78 +68:38:01.5 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:51.78 +68:38:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:42.93 +68:16:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:31.76 +70:42:24.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.48 05:07:45.90 +67:09:35.1
144.18614 15.61868 galactic Cam Second-epoch detections are separated by 1.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 482905201981198976 | 05:07:40.85 +67:09:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.055 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 482905201981198976,2461093.7619,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482905201981198976 20260222.2619 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:45.90 +67:09:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.62 04:56:44.43 +72:01:23.4
139.43324 17.57318 galactic Cam Second-epoch detections are separated by 1.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:44.43 +72:01:23.4 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.054 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:44.43 +72:01:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:01.71 +73:12:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 05:33:37.30 +66:55:17.6
145.75476 17.65594 galactic Cam Second-epoch detections are separated by 1.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.4041+66.9221 | 05:33:43.61 +66:54:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.4041+66.9221,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.4041+66.9221 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:37.30 +66:55:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 05:16:19.21 +70:07:06.3
142.01696 17.86447 galactic Cam Second-epoch detections are separated by 0.7" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:16:19.21 +70:07:06.3 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.057 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:19.21 +70:07:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483726983843163264,2461093.7619,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483726983843163264 20260222.2619 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:52.44 +67:32:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.60 04:58:25.34 +68:15:17.1
142.72830 15.51270 galactic Cam Second-epoch detections are separated by 2.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:25.34 +68:15:17.1 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.045 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:25.34 +68:15:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.53 04:49:28.13 +70:57:34.3
139.97931 16.48164 galactic Cam Second-epoch detections are separated by 0.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:49:28.13 +70:57:34.3 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.043 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:28.13 +70:57:34.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.68 05:08:23.69 +65:16:32.4
145.84223 14.61976 galactic Cam Second-epoch detections are separated by 1.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:08:23.69 +65:16:32.4 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:23.69 +65:16:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:44.36 +69:13:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 485640786910087296,2461093.7619,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485640786910087296 20260222.2619 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:20.33 +69:34:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.54 04:33:08.27 +68:37:18.6
140.94401 13.91642 galactic Cam Second-epoch detections are separated by 2.5" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:33:08.27 +68:37:18.6 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.049 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:08.27 +68:37:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:59.07 +74:40:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:55.20 +74:25:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483147816093873152,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483147816093873152 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:40.66 +66:13:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 04:51:42.42 +67:55:04.1
142.62511 14.80832 galactic Cam Second-epoch detections are separated by 1.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:51:42.42 +67:55:04.1 (user input) | T | P | (position from user input) J-Ks=0.613+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:42.42 +67:55:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.79 05:21:48.23 +66:01:58.5
145.95176 16.19175 galactic Cam Second-epoch detections are separated by 3.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:48.23 +66:01:58.5 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.047 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:48.23 +66:01:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.65 05:34:31.86 +73:08:44.5
139.93471 20.57431 galactic Cam Second-epoch detections are separated by 1.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:31.86 +73:08:44.5 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.042 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:31.86 +73:08:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.60 05:04:54.25 +70:09:42.7
141.43367 17.06936 galactic Cam Second-epoch detections are separated by 6.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:04:54.25 +70:09:42.7 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.053 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:54.25 +70:09:42.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:56.00 +66:59:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:00.37 +71:27:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.72 05:17:28.24 +66:20:48.4
145.43556 15.98257 galactic Cam Second-epoch detections are separated by 3.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:28.24 +66:20:48.4 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.051 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:28.24 +66:20:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.57 05:24:14.95 +70:32:23.3
141.98732 18.65309 galactic Cam Second-epoch detections are separated by 3.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:24:14.95 +70:32:23.3 (user input) | T | P | (position from user input) J-Ks=0.261+/-0.053 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:14.95 +70:32:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483095005176245376,2461093.7619,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483095005176245376 20260222.2619 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:53.98 +65:39:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.75 04:59:55.20 +69:07:50.8
142.06677 16.12981 galactic Cam Second-epoch detections are separated by 0.4" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:55.20 +69:07:50.8 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.070 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:55.20 +69:07:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.65 04:22:18.21 +67:30:37.3
141.09011 12.42042 galactic Cam Second-epoch detections are separated by 0.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:22:18.21 +67:30:37.3 (user input) | T | P | (position from user input) J-Ks=0.540+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:18.21 +67:30:37.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.63 05:04:00.03 +67:32:28.1
143.64730 15.53278 galactic Cam Second-epoch detections are separated by 3.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 483723444789916928 | 05:03:54.63 +67:31:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.055 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483723444789916928,2461093.7619,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483723444789916928 20260222.2619 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:00.03 +67:32:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043756.79+675237.6,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043756.79+675237.6 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:56.89 +67:52:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.52 04:45:39.09 +66:39:26.7
143.28138 13.57334 galactic Cam Second-epoch detections are separated by 1.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:45:39.09 +66:39:26.7 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:39.09 +66:39:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.61 04:24:21.73 +69:52:39.8
139.44516 14.17450 galactic Cam Second-epoch detections are separated by 1.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:21.73 +69:52:39.8 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.046 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:21.73 +69:52:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.74 04:21:43.68 +65:21:51.4
142.63248 10.89485 galactic Cam Second-epoch detections are separated by 2.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:21:43.68 +65:21:51.4 (user input) | T | P | (position from user input) J-Ks=0.681+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:43.68 +65:21:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.64 05:10:38.40 +65:36:55.5
145.68438 15.00257 galactic Cam Second-epoch detections are separated by 2.3" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:10:38.40 +65:36:55.5 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:38.40 +65:36:55.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:17.48 +66:43:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 13.71 04:23:46.84 +65:58:22.5
142.33289 11.46823 galactic Cam Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:23:46.84 +65:58:22.5 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7619,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2619 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:46.84 +65:58:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IK Cam,2461093.7619,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IK Cam 20260222.2619 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:04.91 +67:38:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0405390+661955,2461093.7619,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0405390+661955 20260222.2619 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:39.68 +66:19:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2619 2461093.7619 12.98 04:40:50.26 +68:20:36.1
141.63292 14.27635 galactic Cam Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 | 04:40:50.26 +68:20:36.1 (user input) | 495853463226964352 (VSX @ VizieR) | CV (VSX @ VizieR) | (position from user input) J-Ks=0.453+/-0.059 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461093.7619,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20260222.2619 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:50.26 +68:20:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0503015+691635,2461093.7619,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0503015+691635 20260222.2619 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:01.52 +69:16:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0433225+695613,2461093.7619,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0433225+695613 20260222.2619 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:22.76 +69:56:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20_00sec_-14_90C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461093.76214027 22.02.2026 06:17:18.919 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 243
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17681
Objects passed selection criteria: 17651
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 15819
Average stars matched: 14962 (94.5825 %)
Memory usage VmPeak: 123684 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:32:11 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461093.76214027 22.02.2026 06:17:18.919 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1510
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 66 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 115055
Objects passed selection criteria: 114789
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 102827
Average stars matched: 97803 (95.1141 %)
Memory usage VmPeak: 2001612 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:35:25 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Cam-06-Q2b1x1
#######################################
########### Starting Cam-06-Q2b1x1 ###########
Processing Cam-06-Q2b1x1
server tau has sufficient free disk space available: 1040363 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1040363 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.png' -> 'transient_report/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits_preview.png'
Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
renamed 'Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.png' -> 'transient_report/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits_preview.png'
Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 616.8181
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 663.8512
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1095.8979
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 666.5822
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1096.0636
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 665.8686
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.7767
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
No bad regions file found ../bad_region.lst
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461093.76158431
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits'
wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:36.020 +70:01:26.51
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:34.011 +70:01:32.16
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:36.020 +70:01:26.51
Second-epoch second image center 04:47:34.011 +70:01:32.16
Angular distance between the image centers 0.00326 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.Vz8iTjvUvv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.RYSGgKN719
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits &> /tmp/tmp.M9tCIyxpl7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits &> /tmp/tmp.w51CsXKhDY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 58 out of 16183 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 233 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.5 pix Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
2.5 pix Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.0 mag. Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
15.0 mag. Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Vz8iTjvUvv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1300, passed=16183
Got 16183 stars (including 14865 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 16183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 292 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 360 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.02"
Estimated accuracy of the plate solution: 5.56"
Excluding outliers - 323 stars left (next iteration limit 245)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RYSGgKN719 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1282, passed=16167
Got 16167 stars (including 14867 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 16167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.M9tCIyxpl7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1443, passed=15653
Got 15653 stars (including 14206 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 15653 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits -region wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.w51CsXKhDY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1436, passed=15583
Got 15583 stars (including 14139 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 15583 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits -region wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out21046.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out21029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21546.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 39s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21026_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21026_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 21029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21032_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 21032_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21033_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21033_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:31.70 +73:15:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.466 500992133896844160 072.63163341498 +73.26538940877 12.0940 11.3376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:35:25.20 +72:03:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.066 498507134538498048 083.85773222768 +72.05237071573 12.3021 11.8045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21040_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21040_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:11:46.45 +71:39:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 5.412 543894115539708672 047.94799231837 +71.65560097475 10.6603 10.1177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:18:14.43 +70:14:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.980 541468936487188992 049.55703929812 +70.24960459289 10.6685 10.1795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21046_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21046_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:19:57.18 +69:34:39.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21047_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21047_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21051_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21051_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21052_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 21052_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21053_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 21053_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21057_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21057_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:07:20.62 +72:59:02.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21388_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21388_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:01.33 +69:06:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 0.496 496311856496236800 071.00549774881 +69.10413684241 12.0561 11.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:54:25.67 +69:35:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.122 496304984544663168 073.60700128984 +69.59244696143 12.0245 11.5664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21409_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21409_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:11:44.51 +74:10:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 0.833 502592954106923136 077.93461430026 +74.17674655585 11.7984 11.3427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21410_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21410_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:54.11 +71:27:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.315 500535802212355456 069.47518647410 +71.45454129490 11.9885 11.5352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21421_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21421_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:20.71 +68:09:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.901 495967984234117504 072.58584113756 +68.15164736946 12.0959 11.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:21.90 +69:39:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.909 496309657472523264 073.34089644158 +69.66338715258 12.1163 11.5643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:20:10.34 +71:33:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.388 498147899176343936 080.04274431906 +71.56495450163 11.8098 11.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:39:26.03 +69:07:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.124 495949120738139392 069.85840946277 +69.12685914197 11.7491 10.8212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21453_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21453_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:58:29.10 +70:11:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.547 496466986416075008 074.62084971996 +70.19715214814 12.1331 11.6663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:03:01.58 +69:16:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.418 496152564748485760 075.75678653403 +69.27565881537 12.0776 10.7438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:04:24.21 +69:47:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.780 496231587848912128 076.10027246800 +69.79728243252 12.0807 11.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21501_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21501_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:01:19.16 +69:55:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.392 496420879945504896 075.32986038896 +69.92969170575 12.2963 11.8303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21509_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21509_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:15:02.77 +73:00:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.679 499272768290947328 078.76097407482 +73.01458988992 12.0140 11.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21510_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21510_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 21517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:08:42.11 +70:40:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.665 497961123936904320 077.17528803194 +70.67887022278 12.3427 11.9350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21522_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21522_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:33.41 +69:03:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.598 496085769416751744 073.13874825646 +69.05725488567 12.1207 11.4710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:31.41 +72:48:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.725 500908669794258688 071.13116150341 +72.81009943899 10.8924 9.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21524_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21524_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:06:10.88 +70:43:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.772 498004893946361344 076.54497419017 +70.71995658085 12.2410 11.6920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21530_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21530_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:22.91 +71:04:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.705 497512007797216000 072.84505007083 +71.06969962283 12.3858 11.9670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:01:58.81 +71:18:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.545 497346595717648128 075.49459615061 +71.30466095945 12.2187 11.7120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21539_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21539_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:32:01.11 +70:36:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.541 500075995896040832 068.00420366583 +70.61558256096 11.9811 11.1111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21540_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21540_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:10:23.49 +70:20:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.853 497749811546257024 077.59765711119 +70.34966982300 12.2340 11.7388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21541_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21541_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:38.93 +70:04:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.535 497138311283551360 072.16183443399 +70.07288180074 12.3814 11.9617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21544_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21544_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:55.01 +70:37:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.415 497393879017030400 070.47894793548 +70.62518735170 12.2777 11.7231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21546_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 21546_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 21547_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21547_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:47.33 +70:14:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.867 497226061756783360 073.44696960334 +70.24650470381 12.2945 11.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21548_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21548_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:12:40.69 +71:00:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.535 498035547130074752 078.16909826939 +71.00118738635 12.2555 11.8416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21549_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21549_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:50.08 +69:12:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.101 496131566649487744 074.95859122697 +69.21164758705 12.1717 11.4669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21551_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21551_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:08.32 +70:50:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.028 497280010843832960 074.78412440507 +70.83488989236 12.4739 12.3403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21555_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21555_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:02:21.16 +70:36:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.593 496514196696579840 075.58767465661 +70.60070141701 12.2569 11.4955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21556_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21556_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:38.88 +70:48:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.698 497259734299281792 074.16159061862 +70.80058414549 12.3074 11.8471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:57.46 +69:47:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.455 496357795465930496 073.48929350501 +69.79478566001 12.1988 11.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21562_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21562_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:38.27 +70:03:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.374 496414725254022016 074.90940428375 +70.05649104509 12.0838 11.2416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:20.95 +70:09:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.551 497139754392550272 072.08701185167 +70.15925888778 12.2287 11.4758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21567_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21567_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:34.87 +71:28:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.417 497536364553758848 073.89513558714 +71.46993794051 12.2366 11.5911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21569_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21569_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:42:54.27 +69:57:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.446 497158617888728192 070.72583732154 +69.96651931837 12.1275 11.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21570_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21570_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:11:00.50 +69:27:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.303 485636418925178880 077.75200090036 +69.46130137194 12.1488 11.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21571_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21571_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:06:29.09 +69:47:15.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 21574_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21574_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:07:54.18 +68:57:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 1.020 484111263156537600 076.97587380471 +68.95250210948 12.2883 11.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21576_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21576_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:48.69 +69:09:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.458 496312440611751424 071.20251827398 +69.16415696069 12.3942 11.9054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21577_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21577_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:40:12.98 +71:44:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.168 500549060773340928 070.05406023501 +71.74828728756 12.2674 11.8208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:02.34 +72:03:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.283 500618368662845312 072.75955953712 +72.05135779446 12.1480 11.4254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:37.58 +71:45:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.291 497594299370237568 073.40638137919 +71.75914395014 12.2557 11.7345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21580_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21580_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:26.81 +69:08:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.293 496276981361613696 072.61171430761 +69.13594259722 12.4351 11.9547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21582_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21582_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:42:34.12 +69:14:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.062 495953587504058496 070.64251757471 +69.23618412916 12.4125 11.6772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:31.95 +72:06:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.367 500616405859699328 073.38299739090 +72.10114957228 12.2825 11.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:48.71 +69:06:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.362 496089205390571136 073.20270193578 +69.11606990190 12.0069 11.0908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21587_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21587_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:04:42.42 +69:36:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.789 496208124445342976 076.17628997313 +69.60192734369 12.3813 11.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:48.93 +69:31:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.840 496770352844471040 069.45372612713 +69.52721705564 10.4768 9.0408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21590_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21590_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:16.36 +70:58:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.227 497425558696036736 071.31799425882 +70.97752671959 12.1323 11.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:28.05 +69:58:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.588 497114667484235392 071.61663582280 +69.98186354805 12.3380 11.8402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21592_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21592_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:41.57 +71:05:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.683 497325468777411072 074.17273107280 +71.09510992157 12.3787 11.8981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:39:57.43 +70:47:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.651 497443696338703616 069.98874639383 +70.79180075424 12.3600 11.8681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21597_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21597_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:06.39 +69:21:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.902 496321850881093376 072.02613252075 +69.36237497532 12.3666 11.8477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21598_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21598_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:18:01.29 +71:25:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.218 498144982896305408 079.50519437627 +71.41796369767 12.2549 11.5658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:00:59.73 +73:20:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.609 502441736899623936 075.24850239058 +73.34851992498 12.2344 11.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21602_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21602_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:47:15.96 +71:12:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.605 497482389702838272 071.81700573509 +71.21347378562 12.7198 12.1969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:31.83 +70:22:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.124 497149581277613824 073.13257366458 +70.37510915807 12.3959 11.9480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:26:30.84 +70:48:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.445 497842170522409600 081.62826218615 +70.81498458439 12.1894 11.5327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21608_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21608_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:12.15 +69:39:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.596 496387581060063616 074.05036222369 +69.65761036864 12.2766 11.6111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21612_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21612_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:03.06 +68:29:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.436 495673864873550336 071.01296568804 +68.48936944338 12.0845 11.2424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:42.50 +71:00:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.328 497507884628616960 072.92681742349 +71.00500054874 12.1398 11.3081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21614_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21614_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:49:34.95 +71:13:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.377 497435523019653888 072.39543620633 +71.22583519656 12.2765 11.6435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21615_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21615_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:26.35 +69:55:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.867 496453345599294848 073.85920492759 +69.92918762145 12.3984 11.9245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21617_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21617_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:39.98 +70:29:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.174 497236270896989952 074.16735066734 +70.48323964001 12.5591 12.0987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21618_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21618_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:10:13.03 +70:15:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.985 497746031975046912 077.55387693936 +70.26423494699 12.3917 11.8676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21620_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21620_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:54:52.08 +68:28:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.102 495996915133741056 073.71628902397 +68.47271563003 12.3444 11.9360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21621_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21621_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:02.17 +68:55:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.632 496062714032151168 072.50861773978 +68.93269850869 12.2390 11.5170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:23.85 +69:14:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.684 496279416604214016 073.09896860508 +69.24531850944 12.5368 12.2258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21628_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21628_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:34:36.37 +70:27:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.920 497057939556142592 068.65096265379 +70.46088888729 12.4616 11.9344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:17.07 +68:47:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.463 496019764359394432 073.32102224375 +68.78751196475 12.4584 12.1510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:57:23.05 +71:35:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.957 497562271795396096 074.34614837541 +71.59931926633 12.5082 12.0548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21631_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21631_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:08:02.47 +69:38:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.391 497665698907158144 077.00943249908 +69.64427279837 12.3959 11.9167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:06.35 +68:52:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.722 496068177230739584 073.27616996121 +68.87347699363 12.2226 11.5282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21637_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21637_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:42:42.42 +71:43:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.932 500523089109028480 070.67621954395 +71.72911520977 12.3713 11.8549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:36:28.44 +68:31:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.001 495891774334984320 069.11775207023 +68.51686819920 12.2987 11.5918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21640_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21640_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:40:29.42 +71:10:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.659 500471961818482816 070.12214366524 +71.17514357283 12.1594 11.3479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21641_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21641_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:28.48 +69:07:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.792 495950632566592384 070.36895243302 +69.13188938463 12.4466 11.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21643_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21643_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:02:38.76 +71:50:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.331 499060876082100480 075.66122648607 +71.84956248916 12.1597 11.4049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:36:46.14 +71:08:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.439 500480654832341376 069.19213393264 +71.14817168780 12.2942 11.6936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21646_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21646_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:00:54.92 +69:22:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.658 496181319550664192 075.22864931833 +69.37663479303 12.3442 11.7304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:39.16 +71:39:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.694 500510199908712064 071.66273687048 +71.65799851574 12.3538 11.8506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21650_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21650_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:20:16.74 +70:28:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.549 497808016942672128 080.06946738385 +70.47289740110 12.2985 11.7801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21652_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21652_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:12:17.30 +71:24:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.446 498811355662429952 078.07176847673 +71.41390609970 12.3451 11.8440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:58:21.49 +70:31:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.547 497237194312010880 074.58909240750 +70.52222020419 12.5262 12.1579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21656_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21656_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:57:03.06 +70:51:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.527 497260524573262848 074.26266990825 +70.86211791494 13.0756 12.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21657_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21657_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:16:26.06 +69:04:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.495 485391949386608640 079.10820516161 +69.07614012477 12.1685 11.4410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21659_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21659_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:00:21.60 +71:26:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.584 497362332477818624 075.08949135950 +71.43956705199 12.5027 12.1290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21660_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21660_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:42.50 +72:14:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.543 500677776650478464 072.17664780260 +72.24884919880 12.3083 11.7766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21662_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21662_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:40.86 +67:39:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.897 483554905975011712 072.16963739096 +67.65214387806 12.3028 11.8159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21663_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21663_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:28:27.53 +70:13:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.685 497039110418991488 067.11453045343 +70.22915273466 12.3368 11.8384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:38:51.27 +68:40:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.129 495900188171441024 069.71357363556 +68.66938618388 12.2979 11.6985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21665_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21665_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:47.32 +70:03:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.525 496988567244388736 069.44674855551 +70.06289114807 12.2930 11.5273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21666_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21666_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:29:02.07 +68:28:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.724 496559177892365568 067.25811379213 +68.47101656546 12.3094 11.7360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:07:18.81 +71:45:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.342 498871416484729856 076.82815525188 +71.75595450693 12.5077 11.7172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21668_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21668_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:12:05.11 +71:14:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.484 498054440688331008 078.02094049010 +71.23860084665 12.3798 11.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21670_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21670_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:22.49 +71:51:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.298 497609756953812352 072.84349751448 +71.85144946063 12.4420 12.0545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21671_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21671_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:19.54 +69:58:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.642 496374494298567808 073.08113399966 +69.96742753119 12.4096 11.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21672_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21672_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:40.96 +70:05:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.462 497165661635014400 071.17034935173 +70.09423570929 12.2371 11.4692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:07:08.99 +70:40:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.765 498002149464552192 076.78708041692 +70.68308850143 12.4285 12.0035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21674_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21674_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:12.66 +70:26:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.542 497244409857070080 073.30241143087 +70.44371015865 12.4468 11.9373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:13:40.40 +67:24:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.255 484436203203883904 078.41815276575 +67.41445742491 12.0905 11.3877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:59.23 +70:29:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.147 497238847877377792 073.99682754357 +70.48362243144 12.4424 11.8519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:27:04.73 +71:08:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.773 497900960034681856 081.76940970576 +71.14024748099 12.2796 11.7669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21683_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21683_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:14.23 +68:26:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.639 496031893347254272 072.05881213719 +68.44957842705 12.3275 11.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21687_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21687_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:24.34 +69:07:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.241 496311238020930944 071.10126733741 +69.11920723194 12.4051 11.8887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21688_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21688_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:54:04.19 +68:28:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.002 495997464889561600 073.51747117237 +68.47855507439 12.6070 12.0909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21691_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21691_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:01:27.44 +70:11:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.304 496439292466951040 075.36410422237 +70.18706085853 12.2950 11.5938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21696_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21696_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:44:55.48 +70:49:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.450 485965933114584320 086.23084630604 +70.83315466861 12.2751 11.7147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:17.68 +68:43:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.747 496020623353178624 073.82311229085 +68.71719919760 12.4118 11.9485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:20:18.64 +71:06:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.362 498073682141265664 080.07752163720 +71.10339443669 12.0887 11.2040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21702_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21702_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:15:14.32 +71:54:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.273 498842279426676352 078.80962649537 +71.90868578077 12.2533 11.5491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21703_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21703_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:58.21 +72:32:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.275 500669594735059968 073.99230224873 +72.53505380897 12.3502 11.7062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21705_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21705_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:50.30 +71:51:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.043 500574937953959040 070.45955079243 +71.86508943939 12.4235 11.9296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:00.30 +70:04:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.489 496379815759185792 073.25087299297 +70.07243277614 12.3503 11.6080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:40:18.36 +68:36:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.083 495872498521972480 070.07654255150 +68.61189954476 12.4286 11.9308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21714_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21714_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:34:44.04 +71:29:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.274 500550572601833984 068.68328374988 +71.49714393593 12.4297 11.8953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:58.58 +71:56:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.497 500625309330102016 071.74402981521 +71.94508159493 12.3485 11.8263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21718_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21718_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:00:56.36 +69:18:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.558 496134006190904576 075.23504475387 +69.31180877250 12.2427 11.4668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21719_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21719_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:13:55.61 +71:38:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.288 498823308553723520 078.48106406365 +71.63976691573 12.3923 11.8855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:09:20.11 +70:42:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.921 497961295735577472 077.33337854352 +70.71613300851 12.4244 11.9268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21722_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21722_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:40:07.84 +70:54:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.635 497457204014485248 070.03228232171 +70.90634609823 12.4473 11.9377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21723_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21723_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:24.50 +70:36:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.422 497253107168786048 073.85173081226 +70.60878335761 12.5893 12.2968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21725_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21725_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:11:32.67 +72:01:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.659 498899930769983488 077.88569103015 +72.02868056850 12.3922 11.8572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21726_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21726_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:42:07.51 +68:10:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.298 495648640526727424 070.53115622067 +68.16768427618 12.1931 11.3543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21728_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21728_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:13:04.57 +70:05:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.471 497681676185329792 078.26866369708 +70.08339385178 12.3135 11.6139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:21.76 +69:43:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.621 496400298462152704 073.84022802915 +69.72916472096 12.2951 11.4052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21732_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21732_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:11:29.78 +70:38:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.213 497946280530110848 077.87395108620 +70.64473821094 12.4014 11.9273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21733_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21733_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:44.33 +70:57:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.494 497285130444817792 074.93452525140 +70.95131802048 12.2855 11.5436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:43:40.83 +72:05:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.554 500595072760599552 070.91982032061 +72.09253887942 12.4226 12.0008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21736_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21736_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:13.80 +68:07:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.579 495636378399092096 070.30736551160 +68.11923621410 12.3883 11.8141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:54.42 +70:00:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.511 497128827995739008 072.72637292854 +70.00655931676 12.4973 11.9679 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21738_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21738_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:54:40.68 +69:23:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.505 496286980045259904 073.66933024428 +69.39001578989 12.4827 12.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21739_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21739_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:47:47.51 +70:45:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.653 497404736694506496 071.94752984756 +70.75236388849 12.5324 12.0262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21741_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21741_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:41.12 +70:21:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.253 496492485639916032 074.92072012262 +70.35103051955 12.5119 12.0065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21742_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21742_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:40.60 +71:16:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.419 497492933843789568 071.16882080913 +71.27821529997 12.2918 11.4978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21744_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21744_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:36:30.69 +69:45:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.096 496787631493876864 069.12779809713 +69.75835921168 12.2464 11.4345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21745_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21745_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:58:22.91 +68:48:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.621 496101574896890752 074.59511410284 +68.80803599710 12.4989 12.0740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21746_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21746_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:29:16.92 +72:33:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.791 498967108355674624 082.31981765076 +72.55016364326 12.4506 11.9900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21748_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21748_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:22.05 +70:20:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.889 497185212326075392 071.09154660590 +70.34280406008 12.5146 11.9761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:15:43.90 +70:53:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.239 497978887921765888 078.93273856022 +70.89980174400 12.1854 11.3041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21752_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21752_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:36:03.95 +70:25:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.878 497058905927793536 069.01604682776 +70.41720124752 12.6331 12.2241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21753_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21753_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:02:48.41 +70:39:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.782 496514991268401792 075.70106993376 +70.66560510551 12.4528 11.9612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21754_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21754_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:58:57.84 +67:55:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.619 483902905703632640 074.74064460806 +67.92010834472 12.3296 11.7577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21755_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21755_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:06:40.43 +71:33:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.566 498854232318249088 076.66814537914 +71.55264973325 12.3145 11.6352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21756_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21756_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:15.61 +70:36:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.606 497206407988245888 072.81469106860 +70.61567736913 12.5173 12.0107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:05.70 +70:05:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.350 497139269056918656 072.02346629828 +70.09296053734 12.3557 11.5662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:29:23.28 +70:20:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.379 497046394683523840 067.34676232422 +70.33517956115 12.3592 11.8435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21759_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21759_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:10:41.65 +70:14:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.146 497745344780277888 077.67347104319 +70.24228268796 12.6541 12.3644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21761_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21761_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:09:20.23 +68:18:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.401 483834254945779072 077.33350261328 +68.30111848653 12.2033 11.4045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:07:57.29 +68:26:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.836 483851366095486720 076.98913033387 +68.43389505167 12.1797 11.4079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21763_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21763_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:44.14 +69:39:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.601 496343364375706368 071.68357964292 +69.65145222599 12.4636 11.8640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21764_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21764_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:11.60 +71:41:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.316 497566120086091008 074.04827557996 +71.68355815387 12.1381 11.2407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21765_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21765_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:39:00.44 +72:57:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.179 500881804776461056 069.75166849942 +72.95323338349 12.1848 11.4186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:42.41 +70:21:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.712 497184520833400576 071.42616545696 +70.35177031487 12.5401 12.0365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21767_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21767_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:01:26.10 +71:15:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.654 497344980809945088 075.35819270838 +71.25966396720 12.4123 11.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:30:51.96 +70:16:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.435 485748298531956480 082.71614200771 +70.27063358881 12.1876 11.3624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21769_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21769_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:48.85 +68:36:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.421 496051336662042752 071.45335927416 +68.60359822391 12.4455 11.9422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21770_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21770_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:59:57.04 +71:54:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.156 497576363586703104 074.98719967321 +71.90900873691 13.2134 12.5604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21771_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21771_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:48:39.25 +70:19:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.621 497193183785273472 072.16303218423 +70.32988048143 12.5187 12.0441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21772_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21772_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:11:55.07 +71:38:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.180 498829875561201792 077.97953420943 +71.63453926278 12.3787 11.7810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:25:26.91 +71:19:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.652 497917658867363712 081.36163644559 +71.31884127069 12.3960 11.9620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:50:31.73 +70:11:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.664 497134703510963968 072.63182840329 +70.18552107674 12.4223 11.7401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:09.89 +70:51:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.494 497421023210229248 071.29090899359 +70.85148470956 12.5575 12.0194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:26:50.34 +71:00:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.332 500138397478157696 066.70973988449 +71.01314767260 12.4143 12.0600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21783_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21783_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:16.33 +68:06:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.488 495601675063539968 071.56783123457 +68.11569394734 12.4842 12.0801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21784_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21784_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:13:22.04 +71:34:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.748 498816234745268608 078.34146394051 +71.56992197692 12.4640 12.0234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21785_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21785_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:42.39 +68:58:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.066 496075495854936576 073.92606139431 +68.97607755389 12.4879 11.9910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21787_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21787_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:16.53 +70:54:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.518 497319215305136384 072.81844867520 +70.90184055231 12.3484 11.6023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21788_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21788_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:43:19.69 +70:17:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.348 497186101381366784 070.83177661378 +70.29151884167 12.4436 11.8296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21789_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21789_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:10:55.71 +72:20:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.351 499098774873363456 077.73192032419 +72.34088074560 12.2942 11.5864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21790_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21790_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:38:25.61 +68:22:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.340 495845143870589440 069.60686560711 +68.37151891390 12.4140 11.8639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:39.48 +70:17:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.322 497368620311401728 070.41425765991 +70.28603645769 12.3176 11.5039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21792_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21792_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:03:45.03 +71:10:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.441 497291418276852224 075.93735042365 +71.16730693278 12.3073 11.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:05:03.21 +72:58:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.545 502181702398813312 076.26293915672 +72.96972033691 12.2493 11.5375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21794_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21794_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:49:56.79 +71:11:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.574 497526060930013824 072.48634393730 +71.18604771655 12.3575 11.6302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21796_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21796_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:12.39 +68:46:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.402 495915723072546944 069.30144762826 +68.78196418478 12.0752 11.0879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21797_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21797_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:04:54.05 +73:15:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.624 502261588790454528 076.22486815738 +73.25450391558 12.3310 11.6915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21798_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21798_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:52:21.37 +69:39:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.555 496354973668350464 073.08862335110 +69.66149607929 12.4528 11.8925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21799_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21799_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:34:28.30 +70:55:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.520 500090328204035712 068.61756828342 +70.91708891345 12.3473 11.5932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:55:32.08 +68:46:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.512 496021413627154304 073.88341590068 +68.77797371960 12.3615 11.5997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21802_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21802_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:29.29 +69:46:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.703 496360303726891392 072.87187500577 +69.77824201289 12.5004 11.9629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:34:01.92 +67:20:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.934 495504093406641152 068.50763127984 +67.34252257324 12.3735 11.8398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21804_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21804_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:44:42.74 +69:46:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.894 497093570604883072 071.17785768488 +69.78237452742 12.6323 11.8737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21805_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21805_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:48:57.41 +71:08:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 5.265 495226947755817472 057.23471535141 +71.14121611919 10.7811 9.3759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:35:28.66 +70:22:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.419 497052854314866944 068.86913937858 +70.37201433758 12.6128 12.0863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:03:30.12 +68:31:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.722 484029345242273664 075.87508498508 +68.52546413017 12.5173 12.1698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21809_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21809_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:56:37.46 +67:49:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.716 483898095340327168 074.15561206568 +67.82177225416 12.3417 11.5227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21810_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21810_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:03:53.22 +71:30:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.870 498850418386797568 075.97122761347 +71.51117606564 12.4850 11.9586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21812_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21812_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:52.66 +71:21:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.528 497499427834340352 071.46897108605 +71.35692432754 12.5582 12.1235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21814_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21814_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:42:11.82 +69:09:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.166 495950838725008000 070.54916488994 +69.15160037398 12.5181 12.0345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:49:33.21 +69:41:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.614 496364186377118464 072.38788522929 +69.68732077463 12.4708 11.8449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:32:59.12 +70:40:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.516 500077958698271744 068.24595791292 +70.67421032059 12.5079 11.9931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21820_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21820_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:39:42.55 +68:18:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.483 495830476562211200 069.92709622687 +68.30714082353 12.4210 11.8941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21821_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21821_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:43:29.79 +71:14:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.498 497494381251331456 070.87373736422 +71.23799572717 12.5926 12.3747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21825_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21825_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:32:50.49 +69:14:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.195 496736680301100160 068.21044228843 +69.24207629864 12.4040 11.8196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21827_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21827_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:07.54 +67:57:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.305 483938395015008000 073.28125189267 +67.95747463752 12.4056 11.8198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:40:30.09 +69:50:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.496 496781137503323776 070.12510501265 +69.83676817168 12.5132 11.8838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:05:46.61 +67:40:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.339 483731691127009920 076.44423415894 +67.68176040132 12.4039 11.9147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:59.61 +71:15:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.387 497486199335070080 071.49804479450 +71.25018402328 12.5260 11.9546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21834_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21834_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:39:21.54 +68:21:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.379 495833672017682176 069.84003175929 +68.35103806564 12.3686 11.7873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:53:40.31 +68:21:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.850 483985025477955840 073.41735558144 +68.35575357889 12.5057 11.9493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:51:45.64 +70:05:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.767 497129790068374912 072.93986145629 +70.09504724261 12.5094 11.9928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21844_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21844_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:46:18.82 +69:44:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.558 497095395970418688 071.57825110593 +69.73772722250 12.5680 12.0913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21847_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21847_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:47:00.09 +71:23:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.710 497499191614858624 071.75004002106 +71.38333434927 12.3908 11.6272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:32:27.21 +68:37:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.232 495817591658815744 068.11328370977 +68.62747177038 12.4491 11.9405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21854_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21854_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:05.46 +71:46:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.612 500563702319575424 069.27223697658 +71.76988932341 12.4787 11.9722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:31:26.64 +68:50:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.403 496586047207595648 067.86080136861 +68.83847473300 12.3764 11.7734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21856_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21856_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:47:25.75 +68:06:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.432 495589369978045568 071.85642689104 +68.10703838874 12.7321 11.8838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:41:12.10 +71:11:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.387 497471115409911296 070.30010005327 +71.19471596338 12.3553 11.6262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:33:55.38 +72:29:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.171 500842256718150528 068.48060620346 +72.49534117255 12.3989 11.8890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21865_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21865_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:45:00.70 +69:49:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.688 497111235809912704 071.25263507509 +69.82522015476 12.5551 12.0198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:28:14.03 +71:58:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.461 500435815372848512 067.05721841606 +71.98300625473 12.3417 11.5694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:31:01.47 +70:53:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.374 500098299663118080 067.75581511613 +70.89082826650 12.3362 11.5207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21879_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21879_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:43:06.03 +67:42:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.513 495576661174185216 070.77476886158 +67.71135102343 12.1048 11.1758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21887_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21887_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:37:26.40 +68:20:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.165 495839027838599040 069.36003771589 +68.34337705355 12.4329 11.8804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21895_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 21895_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:05:39.63 +66:19:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.425 489951662765298816 061.41315582480 +66.33189216013 11.4097 9.8543 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 45s
Prepared the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:18:48.71 +71:20:47.5
03:20:15.03 +71:53:03.1
03:21:57.40 +68:54:10.0
03:17:36.65 +73:18:06.8
04:49:00.21 +70:52:23.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:36.020 +70:01:26.51
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:34.011 +70:01:32.16
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:36.020 +70:01:26.51
Second-epoch second image center 04:47:34.011 +70:01:32.16
Angular distance between the image centers 0.00326 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.fPGirvFGQh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.GRYghZMLWw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits &> /tmp/tmp.yU1yQxaurh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits &> /tmp/tmp.mVKdA8LtTE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 85 out of 113524 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.485425
a=0.000000 b=1.000000 c=21.485425
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1306 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.3 pix Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
2.3 pix Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
14.0 mag. Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
14.0 mag. Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fPGirvFGQh (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9713, passed=113493
Got 113493 stars (including 103609 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 113493 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 303 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.45"
Estimated accuracy of the plate solution: 5.59"
Excluding outliers - 329 stars left (next iteration limit 266)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GRYghZMLWw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9545, passed=112768
Got 112768 stars (including 103038 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 112768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yU1yQxaurh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=37, blended=10032, passed=93923
Got 93923 stars (including 83793 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 93923 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits -region wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-16-30_20.00sec_-14.90C_LIGHT_0213.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mVKdA8LtTE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=10050, passed=94190
Got 94190 stars (including 84032 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 94190 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Cam-06-Q2b1x1_001804_TTUQ2b1x1_26443_dSZ0q0RC/Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits -region wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out132961.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out132990.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133009.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133051.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133060.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133100.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out133121.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out133268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90043.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 471s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 277s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:56:36.64 +65:09:01.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132962_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132962_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132967_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132967_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132972_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132972_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132981_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132981_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132982_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132982_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:51.81 +72:56:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.915 544261318063064064 049.21397425752 +72.94263492554 13.3465 12.6722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132989_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132989_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:14:46.76 +73:10:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.559 544315091053581440 048.69664477998 +73.16817138101 13.1394 12.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132990_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132990_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:12.10 +69:35:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.192 541200724369335680 050.80070771658 +69.59898189000 13.4575 12.6842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132994_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132994_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:19:06.98 +70:57:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.844 543051198141608704 049.77501025085 +70.95237504462 13.3280 12.6841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132995_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132995_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 132996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 132997_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132997_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:41.82 +71:02:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.005 543031411229068672 050.92403511002 +71.04591375067 13.5702 12.9443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 132998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 132999_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 132999_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:08.35 +70:34:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.989 542815803870958080 051.78725844916 +70.56923805652 13.3063 12.6649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133002_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133002_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133004_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133004_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:11:44.49 +71:53:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.739 543910745652803712 047.93527667893 +71.89071210614 12.7755 12.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133013_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133013_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:02.22 +72:53:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.183 544269628824058880 050.00909342377 +72.89960472954 13.0429 12.3112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133014_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133014_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:32:32.01 +68:51:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.574 494554493317426432 053.13298230660 +68.86319141714 13.7057 13.0177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133015_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133015_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:58.97 +71:46:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.138 543952183497410176 050.49292744000 +71.77533156056 13.3454 12.7698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:07:42.80 +73:08:44.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 133020_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133020_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:31:46.30 +68:04:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.520 492783180085122688 052.94509117499 +68.07435622270 13.3717 12.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133023_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133023_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:33:20.49 +67:25:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.592 492001770914521728 053.33794371772 +67.43025575760 13.4417 12.7786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133025_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133025_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:34:48.11 +66:19:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.973 491685145926168448 053.69981041239 +66.32797817252 13.1679 12.4783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133026_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133026_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133027_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133027_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:24:57.17 +68:36:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.132 493038198063386624 051.24100310081 +68.61397248629 13.3921 12.7895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133028_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133028_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133031_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133031_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133033_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133033_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:07:14.78 +72:55:44.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 133035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:35:38.10 +65:07:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.176 488458903932883072 053.90628323073 +65.13146356656 13.2111 12.5157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133037_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133037_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133041_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133041_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:45:52.46 +65:04:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.388 488317410529558400 056.46869789640 +65.07831871739 13.4240 12.6147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 06:02:31.92 +67:58:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.660 1105449304102684288 090.63348871977 +67.98253509303 14.3848 13.6630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:50.46 +70:21:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.621 542968769128348672 050.21235189725 +70.36757176643 13.0277 12.3922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133046_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133046_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133049_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133049_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:15.68 +71:46:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.432 543951461942903552 050.56147754648 +71.77101013003 12.9909 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133050_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133050_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:30:14.62 +66:35:31.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 133051_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133051_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:40:50.94 +65:05:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.703 488423032366338944 055.21139345373 +65.08511655925 13.1438 12.3813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133052_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133052_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133056_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133056_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:24:11.82 +69:25:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.101 541183269622283520 051.04853295943 +69.42195115646 13.0978 12.4116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133057_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133057_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133058_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133058_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133060_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133060_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:10.56 +69:16:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.632 541166021033704704 050.04619455926 +69.27208827587 13.1510 12.4987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133062_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133062_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133070_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133070_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133071_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133071_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:45:03.48 +64:30:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.729 287792499943111040 086.26381474052 +64.50525712435 13.9306 13.2015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133076_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133076_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:12.50 +72:04:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.512 543965480716111744 050.80183761372 +72.07013799511 13.3079 12.6419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133077_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133077_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133078_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133078_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133079_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133079_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:41.65 +73:38:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.124 544691089671147776 052.17333653233 +73.63511239615 13.2091 12.6747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133087_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133087_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 133088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133089_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133089_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133092_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133092_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 133093_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133093_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133094_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133094_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:19.98 +69:11:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.336 493126193353081600 051.83297344140 +69.19460780644 13.3709 12.7523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133099_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133099_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:47.67 +68:26:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 3.867 493029539409460736 050.70093895491 +68.43771195875 13.1320 12.4924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133100_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133100_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:12:47.39 +72:21:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.862 544137137672352000 048.19487058368 +72.35409303096 13.0202 12.6839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133101_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133101_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:33.44 +69:58:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.392 542759969296071808 050.38694834560 +69.97480788926 13.1731 12.5307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:14:19.85 +72:27:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.931 544139409712184192 048.58266079918 +72.45906377461 13.0773 12.4188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133103_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133103_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:24:07.70 +70:38:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.090 543001346458105728 051.03634034156 +70.63525128421 13.1927 12.4548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133105_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133105_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:33:18.63 +67:58:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.540 492771910090952704 053.32988822251 +67.96738494222 13.4179 12.7845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133107_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133107_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:44:28.45 +65:02:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.037 488313630958369792 056.11613576815 +65.04596776212 13.1117 12.4588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:36.60 +69:46:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.814 541264358604482304 049.15078942793 +69.76984429336 13.0069 12.3870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133110_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133110_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:12:14.60 +73:10:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.480 544328796292113152 048.05840556047 +73.17400278287 12.7760 12.0537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133114_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133114_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133118_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133118_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133119_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133119_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133120_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133120_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:12:36.63 +72:30:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.521 544155043393141504 048.15303558370 +72.51464635444 12.7076 12.0773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133122_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133122_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 133123_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133123_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:42.15 +67:29:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.576 492741089405533952 051.92542941771 +67.48745909510 13.0106 12.2948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133125_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133125_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133126_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133126_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:37:35.10 +67:20:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.934 491944046554317056 054.39833952583 +67.34244248248 13.1833 12.5257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133127_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133127_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 133128_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133128_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133130_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133130_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:14:26.38 +71:38:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.423 543844809315129216 048.60715445649 +71.63381164953 12.9215 12.2245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133131_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133131_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133136_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133136_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:07:21.31 +72:48:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.025 544223419272066944 046.83500941200 +72.80515632378 12.6359 11.9861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133137_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133137_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133138_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133138_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:15:42.64 +70:12:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.492 541474051789429888 048.92925889381 +70.20694507534 12.8032 12.1578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133140_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133140_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:33:31.90 +73:40:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.508 544507643028006144 053.38365811203 +73.68133562938 13.3999 12.7325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133142_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133142_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133144_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133144_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:44.51 +68:58:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.426 493128254937505920 050.93438630977 +68.98009563729 12.9507 12.3311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133145_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133145_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133146_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133146_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:55.67 +68:41:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.915 493064998659222272 051.98068450834 +68.69101195409 13.1618 12.2880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133147_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133147_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:35:45.38 +66:53:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.767 491893400300122880 053.93948022528 +66.89380810734 13.2250 12.5558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 133150_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133150_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:31.86 +73:37:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.173 544671298461863040 051.63685925011 +73.63206161273 12.9333 12.3820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:50.73 +66:58:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.050 491870825951697792 052.21317149152 +66.97513976399 12.8499 12.2057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133155_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133155_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133157_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133157_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 133158_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133158_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:52.48 +67:22:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.820 492727792187146240 051.96603799162 +67.37609938903 12.9275 12.2002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133159_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133159_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:35:39.82 +67:28:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.927 491990638359534336 053.91453135993 +67.47348648971 13.3393 12.7460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133162_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133162_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 133165_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133165_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:29:12.56 +73:10:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.551 544458680401276032 052.30536782694 +73.17047591304 13.0965 12.5673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133167_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133167_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133171_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133171_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 133172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:13.24 +70:11:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.251 541473158436233216 049.05320522122 +70.19774966398 12.5574 11.8613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133175_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133175_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 133176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133177_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133177_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 133178_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133178_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:08:59.24 +72:54:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.078 544225442198980096 047.24651471496 +72.90101400490 12.4767 11.8072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133183_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133183_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 133186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:19:07.52 +70:43:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.707 542997493870544896 049.77653651092 +70.72588145743 12.7405 12.0447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 133189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:05.89 +73:43:17.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)
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Considering the candidate 133190_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133190_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 133191_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133191_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133194_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133194_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:24:34.86 +68:29:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.851 493034933888314368 051.14247703600 +68.49292128133 12.8489 12.2957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133195_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133195_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:14:26.53 +71:39:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.205 543915212419039744 048.60693100086 +71.65153591350 12.5220 11.8344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133196_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133196_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:25:21.30 +68:00:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.566 492817745981469696 051.34181701842 +68.01473344916 12.7043 12.1592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133199_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133199_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 133201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133203_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133203_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:48.03 +68:39:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.100 493047337753718400 051.95003926240 +68.65485955680 12.8782 12.2147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133204_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133204_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133207_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133207_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133208_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133208_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:59.57 +73:38:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.391 544691845585507328 052.24701011848 +73.63692283957 13.0163 12.4900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133214_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133214_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:18.67 +67:42:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 5.228 492794828036306688 051.83155204657 +67.70510466961 13.0704 12.3458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133215_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133215_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:33:11.73 +67:38:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.633 492007199753127936 053.29936771352 +67.63958701354 13.0052 12.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:30:39.67 +72:17:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.226 543245231880582272 052.66250220004 +72.28867206822 12.9222 12.3000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133225_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133225_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:30:14.86 +69:06:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.590 494575968153601152 052.56386223077 +69.11507969440 12.7930 12.1605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:09.70 +70:10:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.869 542774709623781376 050.78918047002 +70.18191591478 12.8534 12.2370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133227_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133227_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 133228_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133228_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 133230_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133230_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:53.91 +67:26:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.294 492729712034789376 052.22443903522 +67.44866219263 12.8449 12.1092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133232_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133232_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:14.07 +72:16:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.594 543995747347994752 051.81209161098 +72.27486261865 12.5300 11.7626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 133236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:46.53 +72:04:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.550 543977918941222144 050.44817199449 +72.08112631641 12.7055 12.0283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:56.67 +68:22:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.458 493028126362275840 050.73352059860 +68.38120708910 12.6157 12.0670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133241_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133241_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133244_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133244_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 133245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:18:06.53 +71:09:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.645 543069172581349888 049.52487860514 +71.16440186410 12.4766 11.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133246_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133246_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 133248_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133248_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:25:50.62 +68:04:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.038 492818291440306560 051.46270752074 +68.06834786450 12.7316 12.1442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133249_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133249_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:15:11.75 +73:23:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.437 544345396342773504 048.79769581255 +73.39725480279 12.4009 11.6985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133251_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133251_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133252_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133252_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133253_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133253_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 133255_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133255_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133256_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133256_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:19:55.26 +70:08:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.628 541276311495114880 049.98463071027 +70.14289585317 12.6504 12.0829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133257_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133257_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 133260_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133260_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 133262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 133264_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133264_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133265_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133265_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133267_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133267_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 133268_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133268_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 133275_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133275_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133276_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133276_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 133277_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133277_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:17:23.12 +70:53:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 5.320 543044296130844288 049.34185230201 +70.88757354568 12.5182 11.9362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133279_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133279_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133281_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133281_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133283_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133283_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:52.53 +70:41:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.490 543002544751153664 050.96691558908 +70.68651983202 12.7503 12.1705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133285_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133285_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:47.49 +73:13:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.904 544283377015198208 050.45092499382 +73.22835556546 12.5749 11.9892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133289_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133289_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133291_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133291_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133293_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133293_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:43.09 +73:18:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.374 544473008411649280 051.92995275256 +73.30870934029 12.8410 12.2480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133296_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133296_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133297_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133297_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:15.79 +69:00:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 3.859 493120317837870336 051.81870469629 +69.00846775831 12.7468 12.1238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133298_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133298_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133299_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133299_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:18.26 +67:48:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.921 492796511663454208 051.82556719687 +67.80395440908 12.6764 12.0245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133300_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133300_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 133304_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133304_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133305_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133305_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133306_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133306_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:35.48 +67:57:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.506 492813141776781440 051.64550976224 +67.95626089060 12.5951 12.0257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133307_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133307_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133309_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133309_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133310_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133310_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 133311_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133311_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133312_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133312_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:25:50.72 +67:42:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 5.297 492797091481746176 051.45794509177 +67.70706139089 12.4247 11.7339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133314_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133314_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:05.82 +69:44:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.922 541252397117982336 050.52587791534 +69.74763956513 12.5095 11.9384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133317_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133317_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133318_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133318_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 133320_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133320_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 133323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 133324_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133324_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:31:38.71 +67:22:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.205 491979608883310208 052.90967142583 +67.37811432844 12.7591 11.7407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:41:11.58 +65:28:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.897 488572802167098496 055.29497462431 +65.46822254973 12.4105 11.8009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133327_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133327_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133329_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133329_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:11.23 +73:09:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 5.290 544281242414213120 050.30163135439 +73.15202137945 12.4185 11.8460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133332_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133332_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133336_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133336_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133338_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133338_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:59.21 +69:03:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.057 493121451709220992 051.74512517372 +69.05982887019 12.4355 11.7391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133339_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133339_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133340_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133340_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:18:58.37 +70:12:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.223 541465225635448064 049.74171470291 +70.20448341935 12.4787 11.8281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133341_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133341_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:15:42.18 +72:31:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.472 544234414388004352 048.92081193944 +72.52675133670 12.1913 11.5309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133343_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133343_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 133344_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133344_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 133348_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133348_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:31.01 +70:19:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.866 542794294674803712 051.62767727068 +70.32999932761 12.4298 11.7912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133349_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133349_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 133351_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133351_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:59.45 +68:31:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.187 493077604385519616 050.49790402109 +68.52823377501 12.1289 11.5311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133352_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133352_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133356_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133356_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:50.69 +73:10:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 4.368 544282616803747456 050.46485777878 +73.17092959955 12.1135 11.4821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133357_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133357_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133358_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133358_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:57.01 +69:57:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.787 542701278564842752 051.98769210088 +69.95163258114 12.3988 11.7602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 133360_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133360_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133362_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133362_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:48.69 +68:34:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.943 493056889761045376 051.70040044204 +68.56718724849 12.2042 11.6634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133365_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133365_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:31:28.84 +67:41:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 5.210 492738405046759040 052.87358046270 +67.68506019455 12.0740 11.4181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133366_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133366_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 133368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133370_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133370_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 06:18:39.80 +69:54:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.787 1107394271449583744 094.66613840724 +69.90094190861 13.1825 12.5748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133371_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133371_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 133372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 133373_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133373_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 133374_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133374_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:50.82 +73:24:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.743 544673871146138752 050.71486949517 +73.40578620899 12.0223 11.4746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 133376_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133376_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 133377_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133377_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:16.16 +68:59:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.510 493128186217783424 050.81693090976 +68.99174498105 12.0567 11.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133378_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133378_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133380_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133380_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 133381_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133381_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:59.19 +72:35:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.739 544062680119347840 050.75050913176 +72.59689716397 12.2329 11.6010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133383_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133383_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 133384_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133384_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:27.82 +72:59:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.003 544262207119129984 049.11216280157 +72.98375567250 11.9226 11.3054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133385_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133385_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:26:06.82 +68:20:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.486 493018849232153600 051.52660232166 +68.33641778138 12.0718 11.5034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133386_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133386_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133388_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133388_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133389_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133389_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133390_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133390_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133391_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133391_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133392_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133392_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 133394_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133394_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133395_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133395_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 133396_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133396_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133397_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133397_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 133398_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133398_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133401_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133401_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:17:47.76 +70:27:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 5.090 542987258965214464 049.45299270591 +70.46215919549 12.0031 11.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133402_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133402_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:28.42 +72:04:51.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)
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Considering the candidate 133403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:42.28 +72:30:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 4.967 544057633534098944 050.68072516830 +72.50882879755 11.8060 11.2204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133404_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133404_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 133406_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133406_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 133408_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133408_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133409_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133409_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133410_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133410_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:27:42.56 +70:00:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.076 542713411850756480 051.92888246812 +70.01355963459 12.0322 11.4595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 133413_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133413_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 133414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 133415_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133415_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 133417_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133417_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 133418_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133418_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 133419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133420_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133420_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 133421_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133421_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133425_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133425_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 133426_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133426_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133427_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133427_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133431_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133431_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133434_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133434_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:36.97 +67:12:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.165 492628423824188032 052.15250881531 +67.21168132821 11.6807 11.1116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133435_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133435_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133436_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133436_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 133437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:30:57.02 +68:58:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 3.591 494559715997651328 052.73485284476 +68.97958844451 11.8922 11.3575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133440_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133440_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:48.49 +68:20:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 4.137 492851963982029696 052.20456541030 +68.34728432376 11.7603 11.1364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133441_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133441_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 133442_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133442_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:24:07.33 +70:06:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 4.719 542767421061190144 051.02685656190 +70.10184092587 11.6860 11.1104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:09:26.96 +72:56:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 5.111 544225996252401408 047.36708680813 +72.94410155067 11.9823 10.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133446_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133446_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133447_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133447_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 133449_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133449_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133450_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133450_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 133452_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133452_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 133453_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133453_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:15.16 +67:40:46.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)
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Considering the candidate 133454_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133454_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:16.75 +71:13:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 3.174 543090784856751744 050.06708177549 +71.23299329598 11.5045 10.9476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133455_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133455_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133456_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133456_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133457_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133457_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 133458_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133458_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:34:09.78 +66:27:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.435 491689921929759488 053.54100825977 +66.45559068195 11.5336 10.8270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 133460_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133460_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 133461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 133463_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133463_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:57.17 +69:38:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 2.971 541236321058012032 049.23587014166 +69.63919463609 11.2673 10.8442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133465_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133465_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 133466_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133466_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 133467_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133467_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:22:31.14 +71:38:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 4.463 543198846234185856 050.62582022377 +71.64581328408 11.4363 10.9396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133469_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133469_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133470_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133470_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:45:58.97 +68:00:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 0.269 493476112928592512 056.49581401473 +68.00646442643 12.4144 11.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133472_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133472_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:25:55.30 +70:37:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.457 542814360761782784 051.47991222897 +70.62147956481 11.7578 11.2148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133475_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133475_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 133476_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133476_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133479_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133479_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 133481_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133481_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 133482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133483_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133483_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133484_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133484_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:18:47.97 +71:20:46.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133485_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133485_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133486_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133486_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 133487_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133487_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 133488_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133488_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 133491_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133491_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:20:14.66 +71:53:01.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133492_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133492_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133494_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133494_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 133495_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133495_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133498_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133498_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 133503_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133503_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 133504_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133504_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 133505_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133505_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 133507_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133507_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 133509_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133509_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133510_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133510_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 133511_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133511_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 133512_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133512_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133513_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133513_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133514_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133514_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 133516_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133516_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 133518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:23:55.62 +70:37:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 5.484 543001312098371840 050.98590068260 +70.62948527470 10.3398 9.8033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133519_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133519_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 133520_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133520_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:17:39.40 +73:18:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 5.545 544340306804461568 049.40887007424 +73.30282179264 10.0093 9.4379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133521_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133521_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:21:57.20 +68:54:08.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133522_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133522_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133526_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133526_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 133527_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133527_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:28:40.80 +68:44:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.81, MAG_FAINT_SEARCH_LIMIT=10.79)GAIADR2_OUTPUT=# 2.955 493053934823425280 052.16773826166 +68.74748406823 10.0311 9.5441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133528_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133528_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133532_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133532_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:25:55.70 +69:09:12.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133533_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133533_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:12:40.53 +71:33:21.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133565_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133565_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133584_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133584_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:30:48.69 +64:51:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.52, MAG_FAINT_SEARCH_LIMIT=9.50)GAIADR2_OUTPUT=# 0.446 477013468924148736 067.70271900409 +64.86395099587 9.4941 8.8644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 133665_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133665_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 133698_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133698_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 133717_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133717_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 133731_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133731_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 133733_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133733_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 133735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 133740_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133740_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 133745_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133745_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 133751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133752_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133752_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 133768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 133778_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133778_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 133781_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133781_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133785_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133785_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 133789_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133789_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 133793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 133808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 133811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 133813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 133815_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133815_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:35:50.56 +64:53:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 5.347 488440040436618496 053.96211643078 +64.88474084617 10.2531 9.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133818_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133818_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 133819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 133820_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133820_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 133826_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133826_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 133832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 133843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 133849_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133849_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 133858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 133887_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133887_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 133891_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133891_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 133895_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133895_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133901_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133901_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133908_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133908_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133926_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 133926_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 133928_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133928_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 133965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 133970_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133970_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 133998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 134001_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134001_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 134009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134012_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134012_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 134017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:39:49.03 +65:09:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 5.544 488426056023307520 054.95540970197 +65.16116118763 10.7955 10.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 134030_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134030_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 134041_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134041_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 134044_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134044_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 134056_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134056_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 134058_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134058_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 134059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134064_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134064_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 134074_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134074_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 134085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134090_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134090_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 134094_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134094_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 134095_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134095_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134098_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134098_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 134099_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134099_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 134102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134104_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134104_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 134109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 134110_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134110_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 134118_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134118_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:38:02.15 +64:42:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 5.508 488376234402879744 054.50981924856 +64.70584621252 10.8105 10.2432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134127_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134127_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 134128_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134128_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 134151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 134170_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134170_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 134188_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134188_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134192_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134192_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 134193_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134193_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134194_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134194_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134195_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134195_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134199_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134199_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 134226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134230_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134230_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 134231_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134231_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134242_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134242_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134243_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134243_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134253_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134253_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 134265_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134265_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 134274_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134274_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134280_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134280_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134287_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134287_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134294_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134294_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134301_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134301_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 134315_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134315_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 134316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 134336_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134336_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 134350_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134350_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 134353_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134353_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 134359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 134368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134377_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134377_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134393_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134393_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 134400_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134400_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 134403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 134407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 134411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134415_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134415_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 134419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 134429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 134459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:41:24.44 +65:10:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 4.857 488517521643401856 055.35320228900 +65.17335948873 11.4464 10.8216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134465_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134465_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134469_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134469_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 134475_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134475_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:13:41.10 +72:09:23.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134493_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134493_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134495_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134495_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134504_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134504_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 134518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 134521_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134521_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 134523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 134525_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134525_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 134534_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134534_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 134536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 134560_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134560_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 134567_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134567_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134570_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134570_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 134588_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134588_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134590_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134590_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 134591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 134603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 134605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:38:32.89 +65:07:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 4.779 488467562587298816 054.63773917404 +65.13279465625 11.7523 11.2176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 134638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 134650_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134650_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 134652_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134652_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 134654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134655_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134655_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 134657_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134657_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 134660_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134660_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 134664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:39:43.97 +64:46:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 5.005 488397984117217280 054.93430982899 +64.76839183846 11.6753 11.1002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 134675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 134676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134692_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134692_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 134700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 134701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 134703_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134703_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134704_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134704_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 134708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134709_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134709_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 134712_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134712_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 134720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 134729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 134737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 134747_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134747_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 134766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 134794_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134794_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 134803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 134806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 134811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 134813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 134817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134818_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134818_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 134831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134837_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134837_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 134843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 134845_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134845_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 134850_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134850_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 134853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 134855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134873_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134873_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134875_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 134875_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 134877_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134877_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 134879_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134879_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 134882_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134882_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 134884_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134884_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 134897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134899_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134899_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 134913_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134913_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 134939_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134939_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 134946_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134946_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 134957_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134957_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 134959_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134959_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134969_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134969_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 134980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 134981_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134981_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 134988_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134988_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 134995_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 134995_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 135000_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135000_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 135008_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135008_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 135017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 135018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135020_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135020_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135030_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135030_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 135035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 135065_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135065_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 135076_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135076_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 135093_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135093_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 135109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135119_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135119_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:37:24.93 +64:44:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 5.212 488388191591829120 054.35433771298 +64.74818414068 11.8970 11.2816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135133_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135133_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 135154_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135154_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135159_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135159_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 135164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135168_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135168_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135170_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135170_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135179_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135179_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135190_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135190_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 135193_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135193_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 135202_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135202_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135204_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135204_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 135210_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135210_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135212_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135212_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 135213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135215_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135215_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 135221_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135221_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135223_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135223_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135244_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135244_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 135245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135248_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135248_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135256_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135256_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135259_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135259_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 135267_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135267_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135278_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135278_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 135283_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135283_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135286_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135286_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135300_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135300_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135321_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135321_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 135323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135323_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135328_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135328_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 135331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135345_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135345_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 135359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 135364_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135364_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 135367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135370_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135370_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 135373_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135373_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 135375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135389_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135389_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 135394_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135394_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 135402_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135402_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 135430_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135430_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135435_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135435_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135436_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135436_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 135444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 135455_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135455_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135462_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135462_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 135478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 135485_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135485_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 135486_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135486_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135497_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135497_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:38:13.61 +64:46:57.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
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Considering the candidate 135506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135508_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135508_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135514_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135514_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 135523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135524_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135524_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135534_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135534_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135550_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135550_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 135578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 135580_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135580_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 135592_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135592_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 135607_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135607_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135611_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135611_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 135622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 135623_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135623_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 135625_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135625_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 135633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135642_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135642_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:35:48.39 +64:57:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 4.751 488444880860369536 053.95332884628 +64.96727215553 12.2210 11.5065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 135664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135664_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 135667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135671_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135671_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135682_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135682_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 135693_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135693_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135711_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135711_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135721_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135721_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135727_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135727_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135736_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135736_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 135737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135737_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135741_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135741_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 135743_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135743_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135751_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 135762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 135763_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135763_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 135765_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135765_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135768_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 135772_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135772_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 135774_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135774_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 135781_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135781_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135797_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135797_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 135799_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135799_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 135800_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135800_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 135801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135815_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135815_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135824_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135824_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 135833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135833_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 135836_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135836_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 135841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 135846_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135846_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 135850_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135850_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 135853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135869_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135869_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 135870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 135872_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135872_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 135874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 135878_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135878_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 135881_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135881_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135888_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135888_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 135890_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135890_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 135898_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135898_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135917_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135917_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 135924_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135924_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:10:27.63 +66:37:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.079 489586998563101824 062.61513626809 +66.62532740548 12.1607 10.5140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135934_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135934_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 135947_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135947_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135951_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135951_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135952_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135952_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135954_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 135954_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 135965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 135967_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135967_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 135973_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135973_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 135975_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135975_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 135976_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135976_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 135983_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135983_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 135992_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 135992_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 136003_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136003_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 136009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136009_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 136014_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136014_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 136037_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136037_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136044_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136044_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 136059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136071_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136071_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 136072_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136072_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 136085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136085_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 136086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136089_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136089_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 136100_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136100_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 136106_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136106_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 136109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 136111_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136111_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136120_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136120_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 136121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136121_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136123_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136123_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 136135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 136149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136153_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136153_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136157_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136157_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 136162_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136162_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 136176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 136185_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136185_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 136201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 136203_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136203_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 136209_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136209_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 136218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136218_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 136222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 136225_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136225_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 136233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 136245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 136247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 136258_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136258_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:17:16.85 +66:57:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.926 489701042833419648 064.31682306768 +66.96573963736 12.3157 10.3326 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136263_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136263_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 136268_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136268_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 136277_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136277_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 136279_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136279_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 136288_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136288_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136291_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136291_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 136313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136315_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136315_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136320_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136320_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136321_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136321_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 06:20:44.77 +72:07:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.412 1113727630225334912 095.18689061982 +72.11776271323 13.6861 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136328_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136328_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 136331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 136333_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136333_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 136351_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136351_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 136354_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136354_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:37:35.22 +64:44:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.662 488388500829470336 054.39619165751 +64.75066190031 13.0329 12.3120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136355_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136355_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 136366_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136366_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 136369_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136369_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 136375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 136382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 136386_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136386_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 136401_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136401_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136404_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136404_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 136407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 136411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 136418_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136418_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 136425_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136425_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 136429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136429_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136430_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136430_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136438_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136438_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136443_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136444_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 136447_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136447_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136456_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136456_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 136461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136474_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 136477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 136479_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136479_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 136481_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136481_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136488_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136488_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136490_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136490_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 136494_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136494_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 136501_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136501_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 136507_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136507_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:54:15.75 +66:22:18.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136513_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136513_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 136529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 136535_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136535_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 136541_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136541_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 136556_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136556_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136557_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136557_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 136561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 136566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 136572_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136572_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136573_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136573_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 136583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 136585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 136591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136591_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 136599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 136603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136603_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136610_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136610_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 136619_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136619_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 136630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136630_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136638_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136640_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136640_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136647_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 136667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 136673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136675_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 136691_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136691_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 136694_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136694_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 136705_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136705_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136707_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136707_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 136708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136708_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 136709_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136709_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 136715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 136724_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136724_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 136730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136731_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136731_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 136735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136735_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 136744_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136744_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 136748_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136748_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 136758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136758_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136759_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136759_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 136764_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136764_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 136776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 136780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136795_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136795_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 136801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136801_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 136802_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136802_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 136811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136811_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 136814_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136814_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 136817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136817_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 136823_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136823_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136829_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136829_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 136830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 136838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136838_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 05:09:35.62 +64:54:05.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136849_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136849_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:16:05.48 +70:04:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.010 541460312192666752 049.02376390953 +70.07954948465 12.9123 12.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136851_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136851_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 136852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 136858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136858_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 136869_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136869_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 136885_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136885_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 136889_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136889_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 136897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 136921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 136930_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136930_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 136936_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136936_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 136952_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136952_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 136954_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136954_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 136957_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136957_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 136958_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136958_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136959_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136959_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 136962_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136962_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 136965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 136968_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136968_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 136972_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136972_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 136975_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136975_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 136980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136980_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 136984_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136984_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 136991_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 136991_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 136992_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136992_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 136993_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136993_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 136996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 136996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 137011_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137011_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 137017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137023_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137023_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 137032_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137032_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 137035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137035_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 137036_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137036_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 137042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137042_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137054_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137054_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 137064_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137064_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 137080_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137080_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 137081_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137081_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137084_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137084_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 137086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137086_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137087_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137087_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 137092_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137092_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 137096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137101_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137101_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 137102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137102_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 137104_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137104_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 137106_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137106_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 137109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137109_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 137117_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137117_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137129_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137129_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137130_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137130_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 137132_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137132_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 137134_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137134_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 137135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137135_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 137141_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137141_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137148_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 137149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 137152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137152_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 137154_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137154_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 137167_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137167_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 137171_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137171_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 137175_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137175_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137176_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 137180_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137180_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 137182_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137182_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 137183_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137183_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 137189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137189_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 137213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 137214_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137214_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137231_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137231_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 137236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 137238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 137245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137245_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 137246_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137246_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 137254_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137254_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 137262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 137275_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137275_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137286_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137286_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 137290_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137290_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 137303_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137303_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 137304_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137304_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137313_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 137324_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137324_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 137325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 137329_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137329_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 137330_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137330_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 137334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137337_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 137339_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137339_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 137340_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137340_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137341_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137341_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 137346_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137346_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 137356_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137356_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 137359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 137360_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137360_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 137361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 137372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137372_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137375_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 137376_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137376_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 137380_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137380_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137382_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 137387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 137390_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137390_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 137403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137403_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 137405_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137405_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 137414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137416_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 137424_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137424_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 137440_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137440_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 137448_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137448_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 137459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137459_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 137463_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137463_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 137464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137464_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 137468_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137468_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 137471_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137471_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 137472_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137472_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 137480_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137480_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 137482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137482_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 137484_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137484_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137492_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137492_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137496_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137496_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 137499_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137499_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 137502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137502_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 137508_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137508_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 137517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137517_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 137518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137518_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137520_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137520_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 137523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137523_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 137535_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137535_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137547_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137547_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 137552_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137552_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 137553_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137553_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 137557_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137557_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 137561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137561_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137586_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137586_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 137588_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137588_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137589_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 137598_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137598_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 137599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137599_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 137600_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137600_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 137606_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137606_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 137615_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137615_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 137622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137622_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137629_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137635_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137635_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137636_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137636_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137637_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137637_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:36:43.20 +64:53:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.224 488393620430061696 054.17903266168 +64.88655845606 12.8101 12.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 137645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137645_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 137648_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137648_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 137653_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137653_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 137654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137662_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137662_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 137676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137676_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137677_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137677_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137681_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137685_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137685_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 137694_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137694_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137695_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137695_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 137697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137699_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137699_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 137710_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137710_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 137713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 137715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137715_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 137725_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137725_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 137727_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137727_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137730_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 137742_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137742_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 137757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137766_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:36:47.34 +64:58:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.655 488441517905305600 054.19839486445 +64.98386567435 13.1383 12.5025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 137767_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137767_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 137774_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137774_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137779_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137791_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 137792_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137792_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 137803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137803_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 137807_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137807_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137808_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137819_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137829_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137829_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137830_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137831_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137835_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137835_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 137840_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137840_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 137843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137843_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 137852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137852_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137853_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137855_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 137857_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137857_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137859_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 137874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137874_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 137875_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137875_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 137880_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137880_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137886_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137886_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 137888_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137888_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 137889_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137889_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 137896_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137896_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137898_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137898_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137903_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137903_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137926_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137926_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137927_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137927_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137928_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137928_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 137937_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137937_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137938_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137938_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137942_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137942_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137948_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 137950_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137950_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137951_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137951_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137965_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 137969_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137969_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137971_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 137971_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 137974_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137974_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 137979_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137979_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 137990_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137990_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 137996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137996_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 137998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 137998_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 138004_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138004_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 138005_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138005_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138011_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138011_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138016_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138016_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138017_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 138018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138018_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138028_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138028_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138029_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 138034_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138034_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 138036_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138036_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138038_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 138040_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138040_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 138048_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138048_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 138059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138059_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 138072_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138072_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 138073_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138073_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 138075_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138075_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138077_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138077_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138080_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138080_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 138088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138088_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138090_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138090_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 138098_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138098_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138103_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138103_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 138105_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138105_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 138116_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138116_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138126_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138126_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 138144_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138144_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 138145_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138145_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 138151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138151_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138153_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138153_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 138161_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138161_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138164_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 138166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138166_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 138172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138172_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 138173_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138173_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138186_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 138187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138187_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138197_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138197_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 138201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138201_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 138202_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138202_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 138206_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138206_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138209_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138209_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 138213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138213_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 138216_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138216_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138221_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138221_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 138222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138222_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138226_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 138232_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138232_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 138233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138233_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138234_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138234_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 138235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138235_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138236_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138238_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138243_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138243_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 138247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138247_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 138252_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138252_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 138260_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138260_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 138261_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138261_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 138262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138262_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 138270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138270_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 138271_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138271_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 138280_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138280_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138281_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138281_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 138284_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138284_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138285_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138285_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 138290_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138290_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138293_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138293_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 138295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138295_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 138299_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138299_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138302_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 138305_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138305_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138316_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138319_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 138325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138325_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138326_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138327_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138327_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138330_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138330_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138331_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138334_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138335_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138335_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 138343_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138343_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 138359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138359_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 138361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138361_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138367_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138368_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 138369_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138369_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 138378_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138378_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138387_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 138399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138399_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138407_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 138411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138411_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138414_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138419_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138426_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138426_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138428_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138437_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:09:33.35 +67:08:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.418 490364460661824384 062.38810030451 +67.14629341569 14.5131 13.5144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 138446_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138446_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138458_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138458_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138461_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 138466_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138466_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138471_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138471_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138477_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 138478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138478_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138480_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138480_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138496_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138496_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138498_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138498_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138506_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138515_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138515_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138529_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138531_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 138532_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138532_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 138536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138536_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:17:29.70 +67:32:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.409 490483792033360640 064.37209486686 +67.54071905091 14.4360 13.4740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 138537_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138537_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 138538_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138538_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138543_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138543_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138551_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138551_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 03:34:48.14 +65:14:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 138553_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138553_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138559_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138559_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138562_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138562_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 138565_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138565_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138566_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138569_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138569_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138578_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138579_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 138582_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138582_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138583_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 138585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138585_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138586_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138586_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138593_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 138601_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138601_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 138602_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138602_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 138605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138605_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138613_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138627_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138631_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138631_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138633_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 138634_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138634_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138641_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138641_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:24:05.98 +65:25:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.948 477311986330592896 066.02496824628 +65.42945933328 14.5915 13.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 138643_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138643_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 138646_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138646_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138654_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 138655_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138655_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138658_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138658_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138667_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138672_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138672_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 138673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138673_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138680_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138680_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138686_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138686_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138689_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138689_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138692_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138692_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 138697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138697_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138700_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 138702_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138702_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138713_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138714_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138714_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138721_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138721_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138722_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138722_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 138728_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138728_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138729_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138747_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138747_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 138749_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138749_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138756_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138756_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138757_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 138762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138762_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138769_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138769_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138775_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138775_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138776_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138780_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 138782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138782_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138786_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138786_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 138795_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138795_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 138796_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138796_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 138806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138806_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138807_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138807_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 138810_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138810_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138813_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138827_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138827_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 138840_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138840_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 138841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138841_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138851_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138851_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138870_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138878_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138878_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138881_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138881_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 138886_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138886_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 138893_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138893_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138894_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138894_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 138897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138897_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138903_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138903_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 138908_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138908_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138920_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138920_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 138921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 138921_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 138927_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138927_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 138937_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138937_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 138938_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138938_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 138941_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138941_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 138961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138961_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 138979_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 138979_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:21:55.59 +65:02:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.293 477163139942578816 065.48099096975 +65.04778807924 14.3731 13.2667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 139034_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 139034_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 139039_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 139039_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
**** FOUND 04:12:32.32 +65:34:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.589 489280342196558336 063.13421981403 +65.57029819904 14.4929 13.3659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 139045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 139045_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 77457_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 77457_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 34149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 34149_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 90043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 90043_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
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Considering the candidate 130793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 130793_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111146_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 111146_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 18720_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64860_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 64860_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62200_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 62200_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 07096_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86062_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 86062_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 67832_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
The candidate 28679_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
Preparing report for the candidate 58701_Cam-06-Q2b1x1_2026-02-22_00-17-18_20.00sec_-14.90C_LIGHT_0214
make_report_in_HTML.sh Phase 2 (HTML assembly): 101s
make_report_in_HTML.sh TOTAL: 849s
Prepared the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:18:48.71 +71:20:47.5
03:20:15.03 +71:53:03.1
03:21:57.40 +68:54:10.0
03:17:36.65 +73:18:06.8
04:49:00.21 +70:52:23.8
04:40:50.26 +68:20:36.1
03:23:49.95 +72:24:42.1
03:27:23.44 +73:16:40.5
03:28:24.68 +67:21:36.8
04:54:35.41 +65:43:22.6
05:08:37.97 +67:34:29.7
03:33:23.91 +65:47:14.7
04:59:11.91 +68:56:04.7
04:39:00.14 +66:59:08.5
04:09:29.02 +66:45:48.7
04:49:39.91 +65:30:41.4
04:06:53.12 +66:22:13.5
05:09:24.68 +69:45:20.8
04:28:00.05 +70:46:05.3
04:06:29.37 +70:10:40.9
04:56:36.61 +66:02:19.7
04:26:07.72 +65:11:15.6
03:25:43.28 +68:30:54.2
04:57:14.40 +69:47:59.1
03:39:52.39 +64:49:08.8
05:03:35.97 +68:40:11.3
03:28:05.38 +67:07:18.0
04:57:18.04 +73:03:08.3
03:20:46.63 +71:53:16.4
03:18:15.86 +71:31:05.7
04:34:49.11 +66:05:18.4
03:59:59.86 +72:53:40.8
03:24:15.39 +68:25:18.5
04:24:10.30 +70:35:42.2
03:23:44.73 +69:23:58.9
03:13:48.96 +71:16:02.0
03:28:27.76 +67:16:28.9
03:20:35.25 +73:42:58.0
04:33:53.77 +67:52:43.2
03:19:56.56 +70:59:48.9
06:09:53.99 +68:10:40.9
04:40:37.36 +66:51:38.7
03:21:12.84 +72:04:33.5
03:24:07.24 +70:13:44.0
03:20:53.48 +70:34:05.8
03:27:34.46 +67:15:09.2
03:40:04.83 +64:57:22.5
03:17:00.40 +70:50:19.7
03:19:58.99 +69:16:23.3
03:18:33.74 +71:46:41.9
04:58:12.36 +68:55:42.1
03:25:46.72 +69:49:37.8
03:26:46.00 +68:32:03.9
03:09:36.37 +72:28:22.0
03:23:18.89 +69:58:47.0
03:23:57.37 +71:26:46.7
03:21:42.86 +72:17:50.9
03:14:43.69 +73:15:53.3
03:24:26.83 +70:50:47.3
03:18:14.36 +70:37:20.7
04:32:07.34 +69:05:37.2
03:24:25.53 +69:38:10.4
05:21:07.22 +73:47:45.2
03:33:08.32 +67:23:34.8
03:26:32.55 +71:04:43.6
03:19:31.94 +72:10:47.9
03:22:25.93 +73:51:49.3
03:34:37.84 +66:02:00.9
04:49:35.97 +70:19:02.2
03:13:43.45 +71:55:12.5
04:40:25.93 +66:00:12.0
03:18:03.49 +72:49:34.1
03:24:59.72 +68:07:51.3
03:20:39.83 +69:14:05.7
03:14:37.63 +71:48:15.1
03:42:11.71 +65:21:10.5
04:51:10.17 +67:30:35.6
03:24:27.13 +69:27:01.7
03:13:47.53 +72:20:15.9
03:23:49.82 +68:53:43.6
03:22:15.19 +72:01:37.7
03:20:52.60 +72:38:20.7
03:21:54.60 +72:12:50.2
03:20:49.92 +73:23:30.7
03:20:42.15 +69:26:29.3
03:13:42.66 +71:26:02.0
03:21:28.85 +72:15:44.2
03:17:17.67 +71:01:34.9
03:22:44.70 +72:13:06.0
03:25:49.03 +69:41:05.1
05:52:27.95 +70:32:03.4
03:25:46.42 +69:34:24.4
03:23:20.24 +73:07:29.1
03:13:23.56 +73:25:48.0
03:20:36.22 +69:40:29.2
04:15:10.34 +68:05:26.0
03:23:10.52 +72:10:59.6
03:16:15.61 +70:14:20.2
06:03:45.46 +69:29:32.8
03:29:58.20 +73:49:29.5
03:25:16.25 +69:12:39.7
04:05:44.65 +69:16:48.3
03:24:18.62 +72:38:27.2
03:19:09.10 +71:46:37.1
03:21:16.18 +72:46:17.9
04:49:40.41 +66:03:58.7
03:32:34.88 +67:07:40.9
03:34:51.75 +66:55:44.1
03:23:09.53 +73:26:44.5
03:32:41.33 +65:47:02.6
03:28:50.03 +67:18:28.0
03:11:45.29 +71:39:17.0
03:36:03.85 +65:41:48.0
04:29:51.41 +65:59:09.4
04:42:14.61 +69:04:10.8
03:35:47.13 +64:54:42.0
03:09:56.56 +72:04:47.6
05:46:27.83 +68:07:42.4
03:37:57.98 +64:58:21.5
04:42:28.43 +68:14:34.9
03:14:32.41 +71:22:49.7
04:18:01.21 +71:13:54.8
03:08:43.76 +72:37:13.7
03:26:52.29 +67:44:42.9
05:32:38.92 +71:28:26.7
03:09:13.36 +73:06:14.4
03:13:18.84 +71:39:25.6
04:29:19.30 +69:15:32.7
04:10:08.78 +68:21:09.3
03:06:41.53 +73:20:49.8
03:15:59.00 +70:17:15.3
03:59:41.43 +70:26:56.0
04:50:22.61 +72:53:49.7
06:00:09.66 +68:03:11.5
04:45:55.60 +68:04:56.1
04:50:16.55 +72:56:16.9
03:15:43.29 +70:14:29.2
03:38:02.44 +65:09:10.1
03:16:53.37 +73:32:41.2
03:12:39.36 +73:32:41.3
04:24:07.66 +66:28:22.4
03:15:09.25 +72:27:59.4
03:11:13.68 +71:48:52.0
05:30:38.77 +74:24:25.9
03:13:02.10 +71:17:23.4
04:55:33.28 +66:54:53.6
04:46:15.03 +66:27:35.9
03:37:10.74 +65:24:41.2
04:56:31.70 +72:51:33.2
04:30:29.66 +69:08:31.8
03:38:04.35 +65:03:18.0
03:12:37.20 +71:01:07.3
03:12:17.32 +71:03:39.3
04:16:55.95 +69:09:50.1
03:35:06.48 +65:31:51.5
03:32:50.35 +66:06:24.3
05:03:33.67 +65:44:41.9
04:38:34.80 +65:24:54.1
03:08:56.28 +72:42:54.3
03:14:52.33 +70:17:28.3
04:20:01.18 +68:13:23.8
04:47:41.80 +69:27:47.0
03:15:35.81 +72:24:24.1
03:16:22.28 +73:26:00.9
04:49:15.36 +71:09:23.7
05:41:41.51 +70:56:51.3
03:35:27.85 +65:16:45.9
04:41:43.29 +68:50:32.3
04:45:29.01 +74:16:14.9
04:53:36.69 +68:12:25.3
05:01:54.70 +71:44:41.0
05:15:55.39 +73:40:00.6
05:07:27.05 +73:55:10.7
04:11:33.52 +65:34:23.1
05:18:29.74 +68:23:54.5
03:17:52.20 +69:28:34.6
05:42:44.09 +73:30:38.5
04:52:20.32 +66:13:58.9
04:41:09.29 +67:50:55.8
05:13:37.00 +68:17:16.8
05:21:14.70 +71:13:30.4
04:46:38.69 +67:36:53.1
03:12:41.44 +71:22:37.7
04:43:33.40 +68:31:39.8
04:24:11.86 +67:34:11.7
04:54:16.80 +65:21:24.4
05:07:59.96 +65:47:23.5
05:44:28.44 +64:32:51.6
05:14:42.86 +74:54:33.0
05:02:51.25 +66:09:46.2
04:58:00.75 +64:59:19.1
06:05:08.07 +67:40:13.1
06:15:00.15 +70:38:30.3
05:01:00.33 +67:24:59.2
05:54:40.37 +71:02:25.3
05:23:14.73 +73:37:18.3
05:29:51.59 +72:20:59.2
04:10:47.07 +70:07:30.0
05:38:34.10 +72:33:43.1
05:08:36.53 +67:53:18.6
04:58:07.28 +67:47:56.5
04:10:46.66 +71:04:07.4
04:37:51.24 +68:09:14.6
04:18:30.24 +65:45:02.5
04:34:09.12 +65:02:33.6
05:34:04.06 +68:50:00.1
05:46:03.79 +71:54:41.3
05:18:32.04 +70:53:23.7
04:58:39.37 +66:34:13.5
05:33:07.50 +73:20:44.2
04:53:10.49 +66:33:43.0
05:35:59.02 +70:13:11.9
04:45:01.40 +66:58:29.5
05:07:54.88 +70:14:26.2
04:39:44.78 +68:25:39.5
05:39:48.94 +69:57:50.5
04:15:10.29 +69:56:54.5
04:59:06.11 +65:22:21.5
05:46:20.74 +71:28:22.1
05:24:14.41 +73:27:32.5
05:23:27.76 +69:02:17.2
04:51:08.18 +69:25:23.5
05:03:50.20 +67:50:15.1
05:54:24.79 +67:33:38.3
05:29:37.95 +70:26:14.1
04:26:02.56 +66:20:55.3
05:30:09.22 +72:28:21.0
05:26:36.97 +71:07:51.0
04:24:34.49 +67:41:11.5
04:15:07.08 +69:52:49.4
05:40:11.87 +69:35:20.3
04:52:47.11 +67:49:23.7
04:56:09.41 +64:58:46.4
04:44:18.83 +65:11:40.3
05:20:36.16 +66:22:27.7
04:56:10.62 +65:17:00.3
06:07:10.88 +71:30:10.1
04:32:38.51 +65:48:33.5
05:14:49.52 +68:54:52.3
05:25:27.29 +68:03:13.0
05:05:57.61 +67:42:12.8
05:27:08.09 +72:06:04.5
05:10:25.35 +72:12:14.9
04:32:40.13 +64:59:59.4
04:12:20.14 +68:01:10.0
04:57:11.50 +68:24:56.5
04:38:02.78 +65:40:20.5
04:36:00.62 +66:19:30.3
04:39:28.54 +68:08:45.8
05:37:58.51 +72:33:47.4
05:15:43.20 +67:43:19.8
05:15:42.78 +70:06:35.3
05:49:03.77 +70:50:50.0
05:25:31.96 +73:04:27.6
05:32:07.06 +69:18:10.7
05:00:51.56 +66:17:45.0
05:03:55.30 +66:34:55.1
06:02:29.94 +73:26:04.8
03:35:57.75 +66:13:34.2
05:40:39.98 +72:33:22.0
05:19:24.42 +67:05:13.2
04:53:12.16 +70:21:09.7
05:25:52.22 +71:45:50.9
05:12:16.01 +71:06:23.0
04:04:56.61 +69:20:11.2
04:32:57.88 +67:16:23.9
04:02:25.46 +66:01:48.3
04:35:48.44 +65:59:27.1
04:42:27.97 +68:36:51.8
05:20:23.77 +66:54:07.5
05:03:25.11 +68:43:25.9
04:59:42.61 +68:55:49.8
04:29:28.68 +69:15:10.9
05:58:11.41 +73:30:51.0
05:28:51.53 +70:26:47.6
05:08:12.10 +70:39:45.2
05:07:06.59 +65:02:37.5
05:17:51.78 +68:38:01.5
05:17:42.93 +68:16:35.1
05:49:31.76 +70:42:24.9
05:07:45.90 +67:09:35.1
04:56:44.43 +72:01:23.4
05:01:01.71 +73:12:34.2
05:33:37.30 +66:55:17.6
05:16:19.21 +70:07:06.3
05:05:52.44 +67:32:38.7
04:58:25.34 +68:15:17.1
04:49:28.13 +70:57:34.3
05:08:23.69 +65:16:32.4
04:44:44.36 +69:13:55.4
05:11:20.33 +69:34:44.2
04:33:08.27 +68:37:18.6
04:56:59.07 +74:40:32.2
04:10:55.20 +74:25:40.5
04:39:40.66 +66:13:36.1
04:51:42.42 +67:55:04.1
05:21:48.23 +66:01:58.5
05:34:31.86 +73:08:44.5
05:04:54.25 +70:09:42.7
05:30:56.00 +66:59:27.2
04:53:00.37 +71:27:22.2
05:17:28.24 +66:20:48.4
05:24:14.95 +70:32:23.3
04:35:53.98 +65:39:43.8
04:59:55.20 +69:07:50.8
04:22:18.21 +67:30:37.3
05:04:00.03 +67:32:28.1
04:37:56.89 +67:52:36.3
04:45:39.09 +66:39:26.7
04:24:21.73 +69:52:39.8
04:21:43.68 +65:21:51.4
05:10:38.40 +65:36:55.5
05:13:17.48 +66:43:01.5
04:23:46.84 +65:58:22.5
04:33:22.76 +69:56:13.2
05:03:01.52 +69:16:32.5
03:41:04.91 +67:38:56.4
04:05:39.68 +66:19:59.2
########### Completed Cam-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
03:18:48.71 +71:20:47.5
03:20:15.03 +71:53:03.1
03:21:57.40 +68:54:10.0
03:17:36.65 +73:18:06.8
04:49:00.21 +70:52:23.8
03:23:49.95 +72:24:42.1
03:27:23.44 +73:16:40.5
03:28:24.68 +67:21:36.8
04:54:35.41 +65:43:22.6
05:08:37.97 +67:34:29.7
03:33:23.91 +65:47:14.7
04:59:11.91 +68:56:04.7
04:39:00.14 +66:59:08.5
04:09:29.02 +66:45:48.7
04:49:39.91 +65:30:41.4
04:06:53.12 +66:22:13.5
05:09:24.68 +69:45:20.8
04:28:00.05 +70:46:05.3
04:06:29.37 +70:10:40.9
04:56:36.61 +66:02:19.7
04:26:07.72 +65:11:15.6
03:25:43.28 +68:30:54.2
04:57:14.40 +69:47:59.1
03:39:52.39 +64:49:08.8
05:03:35.97 +68:40:11.3
03:28:05.38 +67:07:18.0
04:57:18.04 +73:03:08.3
03:20:46.63 +71:53:16.4
03:18:15.86 +71:31:05.7
04:34:49.11 +66:05:18.4
03:59:59.86 +72:53:40.8
03:24:15.39 +68:25:18.5
04:24:10.30 +70:35:42.2
03:23:44.73 +69:23:58.9
03:13:48.96 +71:16:02.0
03:28:27.76 +67:16:28.9
03:20:35.25 +73:42:58.0
04:33:53.77 +67:52:43.2
03:19:56.56 +70:59:48.9
06:09:53.99 +68:10:40.9
04:40:37.36 +66:51:38.7
03:21:12.84 +72:04:33.5
03:24:07.24 +70:13:44.0
03:20:53.48 +70:34:05.8
03:27:34.46 +67:15:09.2
03:40:04.83 +64:57:22.5
03:17:00.40 +70:50:19.7
03:19:58.99 +69:16:23.3
03:18:33.74 +71:46:41.9
04:58:12.36 +68:55:42.1
03:25:46.72 +69:49:37.8
03:26:46.00 +68:32:03.9
03:09:36.37 +72:28:22.0
03:23:18.89 +69:58:47.0
03:23:57.37 +71:26:46.7
03:21:42.86 +72:17:50.9
03:14:43.69 +73:15:53.3
03:24:26.83 +70:50:47.3
03:18:14.36 +70:37:20.7
04:32:07.34 +69:05:37.2
03:24:25.53 +69:38:10.4
05:21:07.22 +73:47:45.2
03:33:08.32 +67:23:34.8
03:26:32.55 +71:04:43.6
03:19:31.94 +72:10:47.9
03:22:25.93 +73:51:49.3
03:34:37.84 +66:02:00.9
04:49:35.97 +70:19:02.2
03:13:43.45 +71:55:12.5
04:40:25.93 +66:00:12.0
03:18:03.49 +72:49:34.1
03:24:59.72 +68:07:51.3
03:20:39.83 +69:14:05.7
03:14:37.63 +71:48:15.1
03:42:11.71 +65:21:10.5
04:51:10.17 +67:30:35.6
03:24:27.13 +69:27:01.7
03:13:47.53 +72:20:15.9
03:23:49.82 +68:53:43.6
03:22:15.19 +72:01:37.7
03:20:52.60 +72:38:20.7
03:21:54.60 +72:12:50.2
03:20:49.92 +73:23:30.7
03:20:42.15 +69:26:29.3
03:13:42.66 +71:26:02.0
03:21:28.85 +72:15:44.2
03:17:17.67 +71:01:34.9
03:22:44.70 +72:13:06.0
03:25:49.03 +69:41:05.1
05:52:27.95 +70:32:03.4
03:25:46.42 +69:34:24.4
03:23:20.24 +73:07:29.1
03:13:23.56 +73:25:48.0
03:20:36.22 +69:40:29.2
04:15:10.34 +68:05:26.0
03:23:10.52 +72:10:59.6
03:16:15.61 +70:14:20.2
06:03:45.46 +69:29:32.8
03:29:58.20 +73:49:29.5
03:25:16.25 +69:12:39.7
04:05:44.65 +69:16:48.3
03:24:18.62 +72:38:27.2
03:19:09.10 +71:46:37.1
03:21:16.18 +72:46:17.9
04:49:40.41 +66:03:58.7
03:32:34.88 +67:07:40.9
03:34:51.75 +66:55:44.1
03:23:09.53 +73:26:44.5
03:32:41.33 +65:47:02.6
03:28:50.03 +67:18:28.0
03:11:45.29 +71:39:17.0
03:36:03.85 +65:41:48.0
04:29:51.41 +65:59:09.4
04:42:14.61 +69:04:10.8
03:35:47.13 +64:54:42.0
03:09:56.56 +72:04:47.6
05:46:27.83 +68:07:42.4
03:37:57.98 +64:58:21.5
04:42:28.43 +68:14:34.9
03:14:32.41 +71:22:49.7
04:18:01.21 +71:13:54.8
03:08:43.76 +72:37:13.7
03:26:52.29 +67:44:42.9
05:32:38.92 +71:28:26.7
03:09:13.36 +73:06:14.4
03:13:18.84 +71:39:25.6
04:29:19.30 +69:15:32.7
04:10:08.78 +68:21:09.3
03:06:41.53 +73:20:49.8
03:15:59.00 +70:17:15.3
03:59:41.43 +70:26:56.0
04:50:22.61 +72:53:49.7
06:00:09.66 +68:03:11.5
04:45:55.60 +68:04:56.1
04:50:16.55 +72:56:16.9
03:15:43.29 +70:14:29.2
03:38:02.44 +65:09:10.1
03:16:53.37 +73:32:41.2
03:12:39.36 +73:32:41.3
04:24:07.66 +66:28:22.4
03:15:09.25 +72:27:59.4
03:11:13.68 +71:48:52.0
05:30:38.77 +74:24:25.9
03:13:02.10 +71:17:23.4
04:55:33.28 +66:54:53.6
04:46:15.03 +66:27:35.9
03:37:10.74 +65:24:41.2
04:56:31.70 +72:51:33.2
04:30:29.66 +69:08:31.8
03:38:04.35 +65:03:18.0
03:12:37.20 +71:01:07.3
03:12:17.32 +71:03:39.3
04:16:55.95 +69:09:50.1
03:35:06.48 +65:31:51.5
03:32:50.35 +66:06:24.3
05:03:33.67 +65:44:41.9
04:38:34.80 +65:24:54.1
03:08:56.28 +72:42:54.3
03:14:52.33 +70:17:28.3
04:20:01.18 +68:13:23.8
04:47:41.80 +69:27:47.0
03:15:35.81 +72:24:24.1
03:16:22.28 +73:26:00.9
04:49:15.36 +71:09:23.7
05:41:41.51 +70:56:51.3
03:35:27.85 +65:16:45.9
04:41:43.29 +68:50:32.3
04:45:29.01 +74:16:14.9
04:53:36.69 +68:12:25.3
05:01:54.70 +71:44:41.0
05:15:55.39 +73:40:00.6
05:07:27.05 +73:55:10.7
04:11:33.52 +65:34:23.1
05:18:29.74 +68:23:54.5
03:17:52.20 +69:28:34.6
05:42:44.09 +73:30:38.5
04:52:20.32 +66:13:58.9
04:41:09.29 +67:50:55.8
05:13:37.00 +68:17:16.8
05:21:14.70 +71:13:30.4
04:46:38.69 +67:36:53.1
03:12:41.44 +71:22:37.7
04:43:33.40 +68:31:39.8
04:24:11.86 +67:34:11.7
04:54:16.80 +65:21:24.4
05:07:59.96 +65:47:23.5
05:44:28.44 +64:32:51.6
05:14:42.86 +74:54:33.0
05:02:51.25 +66:09:46.2
04:58:00.75 +64:59:19.1
06:05:08.07 +67:40:13.1
06:15:00.15 +70:38:30.3
05:01:00.33 +67:24:59.2
05:54:40.37 +71:02:25.3
05:23:14.73 +73:37:18.3
05:29:51.59 +72:20:59.2
04:10:47.07 +70:07:30.0
05:38:34.10 +72:33:43.1
05:08:36.53 +67:53:18.6
04:58:07.28 +67:47:56.5
04:10:46.66 +71:04:07.4
04:37:51.24 +68:09:14.6
04:18:30.24 +65:45:02.5
04:34:09.12 +65:02:33.6
05:34:04.06 +68:50:00.1
05:46:03.79 +71:54:41.3
05:18:32.04 +70:53:23.7
04:58:39.37 +66:34:13.5
05:33:07.50 +73:20:44.2
04:53:10.49 +66:33:43.0
05:35:59.02 +70:13:11.9
04:45:01.40 +66:58:29.5
05:07:54.88 +70:14:26.2
04:39:44.78 +68:25:39.5
05:39:48.94 +69:57:50.5
04:15:10.29 +69:56:54.5
04:59:06.11 +65:22:21.5
05:46:20.74 +71:28:22.1
05:24:14.41 +73:27:32.5
05:23:27.76 +69:02:17.2
04:51:08.18 +69:25:23.5
05:03:50.20 +67:50:15.1
05:54:24.79 +67:33:38.3
05:29:37.95 +70:26:14.1
04:26:02.56 +66:20:55.3
05:30:09.22 +72:28:21.0
05:26:36.97 +71:07:51.0
04:24:34.49 +67:41:11.5
04:15:07.08 +69:52:49.4
05:40:11.87 +69:35:20.3
04:52:47.11 +67:49:23.7
04:56:09.41 +64:58:46.4
04:44:18.83 +65:11:40.3
05:20:36.16 +66:22:27.7
04:56:10.62 +65:17:00.3
06:07:10.88 +71:30:10.1
04:32:38.51 +65:48:33.5
05:14:49.52 +68:54:52.3
05:25:27.29 +68:03:13.0
05:05:57.61 +67:42:12.8
05:27:08.09 +72:06:04.5
05:10:25.35 +72:12:14.9
04:32:40.13 +64:59:59.4
04:12:20.14 +68:01:10.0
04:57:11.50 +68:24:56.5
04:38:02.78 +65:40:20.5
04:36:00.62 +66:19:30.3
04:39:28.54 +68:08:45.8
05:37:58.51 +72:33:47.4
05:15:43.20 +67:43:19.8
05:15:42.78 +70:06:35.3
05:49:03.77 +70:50:50.0
05:25:31.96 +73:04:27.6
05:32:07.06 +69:18:10.7
05:00:51.56 +66:17:45.0
05:03:55.30 +66:34:55.1
06:02:29.94 +73:26:04.8
03:35:57.75 +66:13:34.2
05:40:39.98 +72:33:22.0
05:19:24.42 +67:05:13.2
04:53:12.16 +70:21:09.7
05:25:52.22 +71:45:50.9
05:12:16.01 +71:06:23.0
04:04:56.61 +69:20:11.2
04:32:57.88 +67:16:23.9
04:02:25.46 +66:01:48.3
04:35:48.44 +65:59:27.1
04:42:27.97 +68:36:51.8
05:20:23.77 +66:54:07.5
05:03:25.11 +68:43:25.9
04:59:42.61 +68:55:49.8
04:29:28.68 +69:15:10.9
05:58:11.41 +73:30:51.0
05:28:51.53 +70:26:47.6
05:08:12.10 +70:39:45.2
05:07:06.59 +65:02:37.5
05:17:51.78 +68:38:01.5
05:17:42.93 +68:16:35.1
05:49:31.76 +70:42:24.9
05:07:45.90 +67:09:35.1
04:56:44.43 +72:01:23.4
05:01:01.71 +73:12:34.2
05:33:37.30 +66:55:17.6
05:16:19.21 +70:07:06.3
05:05:52.44 +67:32:38.7
04:58:25.34 +68:15:17.1
04:49:28.13 +70:57:34.3
05:08:23.69 +65:16:32.4
04:44:44.36 +69:13:55.4
05:11:20.33 +69:34:44.2
04:33:08.27 +68:37:18.6
04:56:59.07 +74:40:32.2
04:10:55.20 +74:25:40.5
04:39:40.66 +66:13:36.1
04:51:42.42 +67:55:04.1
05:21:48.23 +66:01:58.5
05:34:31.86 +73:08:44.5
05:04:54.25 +70:09:42.7
05:30:56.00 +66:59:27.2
04:53:00.37 +71:27:22.2
05:17:28.24 +66:20:48.4
05:24:14.95 +70:32:23.3
04:35:53.98 +65:39:43.8
04:59:55.20 +69:07:50.8
04:22:18.21 +67:30:37.3
05:04:00.03 +67:32:28.1
04:37:56.89 +67:52:36.3
04:45:39.09 +66:39:26.7
04:24:21.73 +69:52:39.8
04:21:43.68 +65:21:51.4
05:10:38.40 +65:36:55.5
05:13:17.48 +66:43:01.5
04:23:46.84 +65:58:22.5
03:41:04.91 +67:38:56.4
04:05:39.68 +66:19:59.2
04:40:50.26 +68:20:36.1
05:03:01.52 +69:16:32.5
04:33:22.76 +69:56:13.2
###################################################################################
03:18:48.71 +71:20:47.5 -- not an asteroid (will add it to exclusion list)
03:20:15.03 +71:53:03.1 -- not an asteroid (will add it to exclusion list)
03:21:57.40 +68:54:10.0 -- not an asteroid (will add it to exclusion list)
03:17:36.65 +73:18:06.8 -- not an asteroid (will add it to exclusion list)
04:49:00.21 +70:52:23.8 -- not an asteroid (will add it to exclusion list)
03:23:49.95 +72:24:42.1 -- not an asteroid (will add it to exclusion list)
03:27:23.44 +73:16:40.5 -- not an asteroid (will add it to exclusion list)
03:28:24.68 +67:21:36.8 -- not an asteroid (will add it to exclusion list)
04:54:35.41 +65:43:22.6 -- not an asteroid (will add it to exclusion list)
05:08:37.97 +67:34:29.7 -- not an asteroid (will add it to exclusion list)
03:33:23.91 +65:47:14.7 -- not an asteroid (will add it to exclusion list)
04:59:11.91 +68:56:04.7 -- not an asteroid (will add it to exclusion list)
04:39:00.14 +66:59:08.5 -- not an asteroid (will add it to exclusion list)
04:09:29.02 +66:45:48.7 -- not an asteroid (will add it to exclusion list)
04:49:39.91 +65:30:41.4 -- not an asteroid (will add it to exclusion list)
04:06:53.12 +66:22:13.5 -- not an asteroid (will add it to exclusion list)
05:09:24.68 +69:45:20.8 -- not an asteroid (will add it to exclusion list)
04:28:00.05 +70:46:05.3 -- not an asteroid (will add it to exclusion list)
04:06:29.37 +70:10:40.9 -- not an asteroid (will add it to exclusion list)
04:56:36.61 +66:02:19.7 -- not an asteroid (will add it to exclusion list)
04:26:07.72 +65:11:15.6 -- not an asteroid (will add it to exclusion list)
03:25:43.28 +68:30:54.2 -- not an asteroid (will add it to exclusion list)
04:57:14.40 +69:47:59.1 -- not an asteroid (will add it to exclusion list)
03:39:52.39 +64:49:08.8 -- not an asteroid (will add it to exclusion list)
05:03:35.97 +68:40:11.3 -- not an asteroid (will add it to exclusion list)
03:28:05.38 +67:07:18.0 -- not an asteroid (will add it to exclusion list)
04:57:18.04 +73:03:08.3 -- not an asteroid (will add it to exclusion list)
03:20:46.63 +71:53:16.4 -- not an asteroid (will add it to exclusion list)
03:18:15.86 +71:31:05.7 -- not an asteroid (will add it to exclusion list)
04:34:49.11 +66:05:18.4 -- not an asteroid (will add it to exclusion list)
03:59:59.86 +72:53:40.8 -- not an asteroid (will add it to exclusion list)
03:24:15.39 +68:25:18.5 -- not an asteroid (will add it to exclusion list)
04:24:10.30 +70:35:42.2 -- not an asteroid (will add it to exclusion list)
03:23:44.73 +69:23:58.9 -- not an asteroid (will add it to exclusion list)
03:13:48.96 +71:16:02.0 -- not an asteroid (will add it to exclusion list)
03:28:27.76 +67:16:28.9 -- not an asteroid (will add it to exclusion list)
03:20:35.25 +73:42:58.0 -- not an asteroid (will add it to exclusion list)
04:33:53.77 +67:52:43.2 -- not an asteroid (will add it to exclusion list)
03:19:56.56 +70:59:48.9 -- not an asteroid (will add it to exclusion list)
06:09:53.99 +68:10:40.9 -- not an asteroid (will add it to exclusion list)
04:40:37.36 +66:51:38.7 -- not an asteroid (will add it to exclusion list)
03:21:12.84 +72:04:33.5 -- not an asteroid (will add it to exclusion list)
03:24:07.24 +70:13:44.0 -- not an asteroid (will add it to exclusion list)
03:20:53.48 +70:34:05.8 -- not an asteroid (will add it to exclusion list)
03:27:34.46 +67:15:09.2 -- not an asteroid (will add it to exclusion list)
03:40:04.83 +64:57:22.5 -- not an asteroid (will add it to exclusion list)
03:17:00.40 +70:50:19.7 -- not an asteroid (will add it to exclusion list)
03:19:58.99 +69:16:23.3 -- not an asteroid (will add it to exclusion list)
03:18:33.74 +71:46:41.9 -- not an asteroid (will add it to exclusion list)
04:58:12.36 +68:55:42.1 -- not an asteroid (will add it to exclusion list)
03:25:46.72 +69:49:37.8 -- not an asteroid (will add it to exclusion list)
03:26:46.00 +68:32:03.9 -- not an asteroid (will add it to exclusion list)
03:09:36.37 +72:28:22.0 -- not an asteroid (will add it to exclusion list)
03:23:18.89 +69:58:47.0 -- not an asteroid (will add it to exclusion list)
03:23:57.37 +71:26:46.7 -- not an asteroid (will add it to exclusion list)
03:21:42.86 +72:17:50.9 -- not an asteroid (will add it to exclusion list)
03:14:43.69 +73:15:53.3 -- not an asteroid (will add it to exclusion list)
03:24:26.83 +70:50:47.3 -- not an asteroid (will add it to exclusion list)
03:18:14.36 +70:37:20.7 -- not an asteroid (will add it to exclusion list)
04:32:07.34 +69:05:37.2 -- not an asteroid (will add it to exclusion list)
03:24:25.53 +69:38:10.4 -- not an asteroid (will add it to exclusion list)
05:21:07.22 +73:47:45.2 -- not an asteroid (will add it to exclusion list)
03:33:08.32 +67:23:34.8 -- not an asteroid (will add it to exclusion list)
03:26:32.55 +71:04:43.6 -- not an asteroid (will add it to exclusion list)
03:19:31.94 +72:10:47.9 -- not an asteroid (will add it to exclusion list)
03:22:25.93 +73:51:49.3 -- not an asteroid (will add it to exclusion list)
03:34:37.84 +66:02:00.9 -- not an asteroid (will add it to exclusion list)
04:49:35.97 +70:19:02.2 -- not an asteroid (will add it to exclusion list)
03:13:43.45 +71:55:12.5 -- not an asteroid (will add it to exclusion list)
04:40:25.93 +66:00:12.0 -- not an asteroid (will add it to exclusion list)
03:18:03.49 +72:49:34.1 -- not an asteroid (will add it to exclusion list)
03:24:59.72 +68:07:51.3 -- not an asteroid (will add it to exclusion list)
03:20:39.83 +69:14:05.7 -- not an asteroid (will add it to exclusion list)
03:14:37.63 +71:48:15.1 -- not an asteroid (will add it to exclusion list)
03:42:11.71 +65:21:10.5 -- not an asteroid (will add it to exclusion list)
04:51:10.17 +67:30:35.6 -- not an asteroid (will add it to exclusion list)
03:24:27.13 +69:27:01.7 -- not an asteroid (will add it to exclusion list)
03:13:47.53 +72:20:15.9 -- not an asteroid (will add it to exclusion list)
03:23:49.82 +68:53:43.6 -- not an asteroid (will add it to exclusion list)
03:22:15.19 +72:01:37.7 -- not an asteroid (will add it to exclusion list)
03:20:52.60 +72:38:20.7 -- not an asteroid (will add it to exclusion list)
03:21:54.60 +72:12:50.2 -- not an asteroid (will add it to exclusion list)
03:20:49.92 +73:23:30.7 -- not an asteroid (will add it to exclusion list)
03:20:42.15 +69:26:29.3 -- not an asteroid (will add it to exclusion list)
03:13:42.66 +71:26:02.0 -- not an asteroid (will add it to exclusion list)
03:21:28.85 +72:15:44.2 -- not an asteroid (will add it to exclusion list)
03:17:17.67 +71:01:34.9 -- not an asteroid (will add it to exclusion list)
03:22:44.70 +72:13:06.0 -- not an asteroid (will add it to exclusion list)
03:25:49.03 +69:41:05.1 -- not an asteroid (will add it to exclusion list)
05:52:27.95 +70:32:03.4 -- not an asteroid (will add it to exclusion list)
03:25:46.42 +69:34:24.4 -- not an asteroid (will add it to exclusion list)
03:23:20.24 +73:07:29.1 -- not an asteroid (will add it to exclusion list)
03:13:23.56 +73:25:48.0 -- not an asteroid (will add it to exclusion list)
03:20:36.22 +69:40:29.2 -- not an asteroid (will add it to exclusion list)
04:15:10.34 +68:05:26.0 -- not an asteroid (will add it to exclusion list)
03:23:10.52 +72:10:59.6 -- not an asteroid (will add it to exclusion list)
03:16:15.61 +70:14:20.2 -- not an asteroid (will add it to exclusion list)
06:03:45.46 +69:29:32.8 -- not an asteroid (will add it to exclusion list)
03:29:58.20 +73:49:29.5 -- not an asteroid (will add it to exclusion list)
03:25:16.25 +69:12:39.7 -- not an asteroid (will add it to exclusion list)
04:05:44.65 +69:16:48.3 -- not an asteroid (will add it to exclusion list)
03:24:18.62 +72:38:27.2 -- not an asteroid (will add it to exclusion list)
03:19:09.10 +71:46:37.1 -- not an asteroid (will add it to exclusion list)
03:21:16.18 +72:46:17.9 -- not an asteroid (will add it to exclusion list)
04:49:40.41 +66:03:58.7 -- not an asteroid (will add it to exclusion list)
03:32:34.88 +67:07:40.9 -- not an asteroid (will add it to exclusion list)
03:34:51.75 +66:55:44.1 -- not an asteroid (will add it to exclusion list)
03:23:09.53 +73:26:44.5 -- not an asteroid (will add it to exclusion list)
03:32:41.33 +65:47:02.6 -- not an asteroid (will add it to exclusion list)
03:28:50.03 +67:18:28.0 -- not an asteroid (will add it to exclusion list)
03:11:45.29 +71:39:17.0 -- not an asteroid (will add it to exclusion list)
03:36:03.85 +65:41:48.0 -- not an asteroid (will add it to exclusion list)
04:29:51.41 +65:59:09.4 -- not an asteroid (will add it to exclusion list)
04:42:14.61 +69:04:10.8 -- not an asteroid (will add it to exclusion list)
03:35:47.13 +64:54:42.0 -- not an asteroid (will add it to exclusion list)
03:09:56.56 +72:04:47.6 -- not an asteroid (will add it to exclusion list)
05:46:27.83 +68:07:42.4 -- not an asteroid (will add it to exclusion list)
03:37:57.98 +64:58:21.5 -- not an asteroid (will add it to exclusion list)
04:42:28.43 +68:14:34.9 -- not an asteroid (will add it to exclusion list)
03:14:32.41 +71:22:49.7 -- not an asteroid (will add it to exclusion list)
04:18:01.21 +71:13:54.8 -- not an asteroid (will add it to exclusion list)
03:08:43.76 +72:37:13.7 -- not an asteroid (will add it to exclusion list)
03:26:52.29 +67:44:42.9 -- not an asteroid (will add it to exclusion list)
05:32:38.92 +71:28:26.7 -- not an asteroid (will add it to exclusion list)
03:09:13.36 +73:06:14.4 -- not an asteroid (will add it to exclusion list)
03:13:18.84 +71:39:25.6 -- not an asteroid (will add it to exclusion list)
04:29:19.30 +69:15:32.7 -- not an asteroid (will add it to exclusion list)
04:10:08.78 +68:21:09.3 -- not an asteroid (will add it to exclusion list)
03:06:41.53 +73:20:49.8 -- not an asteroid (will add it to exclusion list)
03:15:59.00 +70:17:15.3 -- not an asteroid (will add it to exclusion list)
03:59:41.43 +70:26:56.0 -- not an asteroid (will add it to exclusion list)
04:50:22.61 +72:53:49.7 -- not an asteroid (will add it to exclusion list)
06:00:09.66 +68:03:11.5 -- not an asteroid (will add it to exclusion list)
04:45:55.60 +68:04:56.1 -- not an asteroid (will add it to exclusion list)
04:50:16.55 +72:56:16.9 -- not an asteroid (will add it to exclusion list)
03:15:43.29 +70:14:29.2 -- not an asteroid (will add it to exclusion list)
03:38:02.44 +65:09:10.1 -- not an asteroid (will add it to exclusion list)
03:16:53.37 +73:32:41.2 -- not an asteroid (will add it to exclusion list)
03:12:39.36 +73:32:41.3 -- not an asteroid (will add it to exclusion list)
04:24:07.66 +66:28:22.4 -- not an asteroid (will add it to exclusion list)
03:15:09.25 +72:27:59.4 -- not an asteroid (will add it to exclusion list)
03:11:13.68 +71:48:52.0 -- not an asteroid (will add it to exclusion list)
05:30:38.77 +74:24:25.9 -- not an asteroid (will add it to exclusion list)
03:13:02.10 +71:17:23.4 -- not an asteroid (will add it to exclusion list)
04:55:33.28 +66:54:53.6 -- not an asteroid (will add it to exclusion list)
04:46:15.03 +66:27:35.9 -- not an asteroid (will add it to exclusion list)
03:37:10.74 +65:24:41.2 -- not an asteroid (will add it to exclusion list)
04:56:31.70 +72:51:33.2 -- not an asteroid (will add it to exclusion list)
04:30:29.66 +69:08:31.8 -- not an asteroid (will add it to exclusion list)
03:38:04.35 +65:03:18.0 -- not an asteroid (will add it to exclusion list)
03:12:37.20 +71:01:07.3 -- not an asteroid (will add it to exclusion list)
03:12:17.32 +71:03:39.3 -- not an asteroid (will add it to exclusion list)
04:16:55.95 +69:09:50.1 -- not an asteroid (will add it to exclusion list)
03:35:06.48 +65:31:51.5 -- not an asteroid (will add it to exclusion list)
03:32:50.35 +66:06:24.3 -- not an asteroid (will add it to exclusion list)
05:03:33.67 +65:44:41.9 -- not an asteroid (will add it to exclusion list)
04:38:34.80 +65:24:54.1 -- not an asteroid (will add it to exclusion list)
03:08:56.28 +72:42:54.3 -- not an asteroid (will add it to exclusion list)
03:14:52.33 +70:17:28.3 -- not an asteroid (will add it to exclusion list)
04:20:01.18 +68:13:23.8 -- not an asteroid (will add it to exclusion list)
04:47:41.80 +69:27:47.0 -- not an asteroid (will add it to exclusion list)
03:15:35.81 +72:24:24.1 -- not an asteroid (will add it to exclusion list)
03:16:22.28 +73:26:00.9 -- not an asteroid (will add it to exclusion list)
04:49:15.36 +71:09:23.7 -- not an asteroid (will add it to exclusion list)
05:41:41.51 +70:56:51.3 -- not an asteroid (will add it to exclusion list)
03:35:27.85 +65:16:45.9 -- not an asteroid (will add it to exclusion list)
04:41:43.29 +68:50:32.3 -- not an asteroid (will add it to exclusion list)
04:45:29.01 +74:16:14.9 -- not an asteroid (will add it to exclusion list)
04:53:36.69 +68:12:25.3 -- not an asteroid (will add it to exclusion list)
05:01:54.70 +71:44:41.0 -- not an asteroid (will add it to exclusion list)
05:15:55.39 +73:40:00.6 -- not an asteroid (will add it to exclusion list)
05:07:27.05 +73:55:10.7 -- not an asteroid (will add it to exclusion list)
04:11:33.52 +65:34:23.1 -- not an asteroid (will add it to exclusion list)
05:18:29.74 +68:23:54.5 -- not an asteroid (will add it to exclusion list)
03:17:52.20 +69:28:34.6 -- not an asteroid (will add it to exclusion list)
05:42:44.09 +73:30:38.5 -- not an asteroid (will add it to exclusion list)
04:52:20.32 +66:13:58.9 -- not an asteroid (will add it to exclusion list)
04:41:09.29 +67:50:55.8 -- not an asteroid (will add it to exclusion list)
05:13:37.00 +68:17:16.8 -- not an asteroid (will add it to exclusion list)
05:21:14.70 +71:13:30.4 -- not an asteroid (will add it to exclusion list)
04:46:38.69 +67:36:53.1 -- not an asteroid (will add it to exclusion list)
03:12:41.44 +71:22:37.7 -- not an asteroid (will add it to exclusion list)
04:43:33.40 +68:31:39.8 -- not an asteroid (will add it to exclusion list)
04:24:11.86 +67:34:11.7 -- not an asteroid (will add it to exclusion list)
04:54:16.80 +65:21:24.4 -- not an asteroid (will add it to exclusion list)
05:07:59.96 +65:47:23.5 -- not an asteroid (will add it to exclusion list)
05:44:28.44 +64:32:51.6 -- not an asteroid (will add it to exclusion list)
05:14:42.86 +74:54:33.0 -- not an asteroid (will add it to exclusion list)
05:02:51.25 +66:09:46.2 -- not an asteroid (will add it to exclusion list)
04:58:00.75 +64:59:19.1 -- not an asteroid (will add it to exclusion list)
06:05:08.07 +67:40:13.1 -- not an asteroid (will add it to exclusion list)
06:15:00.15 +70:38:30.3 -- not an asteroid (will add it to exclusion list)
05:01:00.33 +67:24:59.2 -- not an asteroid (will add it to exclusion list)
05:54:40.37 +71:02:25.3 -- not an asteroid (will add it to exclusion list)
05:23:14.73 +73:37:18.3 -- not an asteroid (will add it to exclusion list)
05:29:51.59 +72:20:59.2 -- not an asteroid (will add it to exclusion list)
04:10:47.07 +70:07:30.0 -- not an asteroid (will add it to exclusion list)
05:38:34.10 +72:33:43.1 -- not an asteroid (will add it to exclusion list)
05:08:36.53 +67:53:18.6 -- not an asteroid (will add it to exclusion list)
04:58:07.28 +67:47:56.5 -- not an asteroid (will add it to exclusion list)
04:10:46.66 +71:04:07.4 -- not an asteroid (will add it to exclusion list)
04:37:51.24 +68:09:14.6 -- not an asteroid (will add it to exclusion list)
04:18:30.24 +65:45:02.5 -- not an asteroid (will add it to exclusion list)
04:34:09.12 +65:02:33.6 -- not an asteroid (will add it to exclusion list)
05:34:04.06 +68:50:00.1 -- not an asteroid (will add it to exclusion list)
05:46:03.79 +71:54:41.3 -- not an asteroid (will add it to exclusion list)
05:18:32.04 +70:53:23.7 -- not an asteroid (will add it to exclusion list)
04:58:39.37 +66:34:13.5 -- not an asteroid (will add it to exclusion list)
05:33:07.50 +73:20:44.2 -- not an asteroid (will add it to exclusion list)
04:53:10.49 +66:33:43.0 -- not an asteroid (will add it to exclusion list)
05:35:59.02 +70:13:11.9 -- not an asteroid (will add it to exclusion list)
04:45:01.40 +66:58:29.5 -- not an asteroid (will add it to exclusion list)
05:07:54.88 +70:14:26.2 -- not an asteroid (will add it to exclusion list)
04:39:44.78 +68:25:39.5 -- not an asteroid (will add it to exclusion list)
05:39:48.94 +69:57:50.5 -- not an asteroid (will add it to exclusion list)
04:15:10.29 +69:56:54.5 -- not an asteroid (will add it to exclusion list)
04:59:06.11 +65:22:21.5 -- not an asteroid (will add it to exclusion list)
05:46:20.74 +71:28:22.1 -- not an asteroid (will add it to exclusion list)
05:24:14.41 +73:27:32.5 -- not an asteroid (will add it to exclusion list)
05:23:27.76 +69:02:17.2 -- not an asteroid (will add it to exclusion list)
04:51:08.18 +69:25:23.5 -- not an asteroid (will add it to exclusion list)
05:03:50.20 +67:50:15.1 -- not an asteroid (will add it to exclusion list)
05:54:24.79 +67:33:38.3 -- not an asteroid (will add it to exclusion list)
05:29:37.95 +70:26:14.1 -- not an asteroid (will add it to exclusion list)
04:26:02.56 +66:20:55.3 -- not an asteroid (will add it to exclusion list)
05:30:09.22 +72:28:21.0 -- not an asteroid (will add it to exclusion list)
05:26:36.97 +71:07:51.0 -- not an asteroid (will add it to exclusion list)
04:24:34.49 +67:41:11.5 -- not an asteroid (will add it to exclusion list)
04:15:07.08 +69:52:49.4 -- not an asteroid (will add it to exclusion list)
05:40:11.87 +69:35:20.3 -- not an asteroid (will add it to exclusion list)
04:52:47.11 +67:49:23.7 -- not an asteroid (will add it to exclusion list)
04:56:09.41 +64:58:46.4 -- not an asteroid (will add it to exclusion list)
04:44:18.83 +65:11:40.3 -- not an asteroid (will add it to exclusion list)
05:20:36.16 +66:22:27.7 -- not an asteroid (will add it to exclusion list)
04:56:10.62 +65:17:00.3 -- not an asteroid (will add it to exclusion list)
06:07:10.88 +71:30:10.1 -- not an asteroid (will add it to exclusion list)
04:32:38.51 +65:48:33.5 -- not an asteroid (will add it to exclusion list)
05:14:49.52 +68:54:52.3 -- not an asteroid (will add it to exclusion list)
05:25:27.29 +68:03:13.0 -- not an asteroid (will add it to exclusion list)
05:05:57.61 +67:42:12.8 -- not an asteroid (will add it to exclusion list)
05:27:08.09 +72:06:04.5 -- not an asteroid (will add it to exclusion list)
05:10:25.35 +72:12:14.9 -- not an asteroid (will add it to exclusion list)
04:32:40.13 +64:59:59.4 -- not an asteroid (will add it to exclusion list)
04:12:20.14 +68:01:10.0 -- not an asteroid (will add it to exclusion list)
04:57:11.50 +68:24:56.5 -- not an asteroid (will add it to exclusion list)
04:38:02.78 +65:40:20.5 -- not an asteroid (will add it to exclusion list)
04:36:00.62 +66:19:30.3 -- not an asteroid (will add it to exclusion list)
04:39:28.54 +68:08:45.8 -- not an asteroid (will add it to exclusion list)
05:37:58.51 +72:33:47.4 -- not an asteroid (will add it to exclusion list)
05:15:43.20 +67:43:19.8 -- not an asteroid (will add it to exclusion list)
05:15:42.78 +70:06:35.3 -- not an asteroid (will add it to exclusion list)
05:49:03.77 +70:50:50.0 -- not an asteroid (will add it to exclusion list)
05:25:31.96 +73:04:27.6 -- not an asteroid (will add it to exclusion list)
05:32:07.06 +69:18:10.7 -- not an asteroid (will add it to exclusion list)
05:00:51.56 +66:17:45.0 -- not an asteroid (will add it to exclusion list)
05:03:55.30 +66:34:55.1 -- not an asteroid (will add it to exclusion list)
06:02:29.94 +73:26:04.8 -- not an asteroid (will add it to exclusion list)
03:35:57.75 +66:13:34.2 -- not an asteroid (will add it to exclusion list)
05:40:39.98 +72:33:22.0 -- not an asteroid (will add it to exclusion list)
05:19:24.42 +67:05:13.2 -- not an asteroid (will add it to exclusion list)
04:53:12.16 +70:21:09.7 -- not an asteroid (will add it to exclusion list)
05:25:52.22 +71:45:50.9 -- not an asteroid (will add it to exclusion list)
05:12:16.01 +71:06:23.0 -- not an asteroid (will add it to exclusion list)
04:04:56.61 +69:20:11.2 -- not an asteroid (will add it to exclusion list)
04:32:57.88 +67:16:23.9 -- not an asteroid (will add it to exclusion list)
04:02:25.46 +66:01:48.3 -- not an asteroid (will add it to exclusion list)
04:35:48.44 +65:59:27.1 -- not an asteroid (will add it to exclusion list)
04:42:27.97 +68:36:51.8 -- not an asteroid (will add it to exclusion list)
05:20:23.77 +66:54:07.5 -- not an asteroid (will add it to exclusion list)
05:03:25.11 +68:43:25.9 -- not an asteroid (will add it to exclusion list)
04:59:42.61 +68:55:49.8 -- not an asteroid (will add it to exclusion list)
04:29:28.68 +69:15:10.9 -- not an asteroid (will add it to exclusion list)
05:58:11.41 +73:30:51.0 -- not an asteroid (will add it to exclusion list)
05:28:51.53 +70:26:47.6 -- not an asteroid (will add it to exclusion list)
05:08:12.10 +70:39:45.2 -- not an asteroid (will add it to exclusion list)
05:07:06.59 +65:02:37.5 -- not an asteroid (will add it to exclusion list)
05:17:51.78 +68:38:01.5 -- not an asteroid (will add it to exclusion list)
05:17:42.93 +68:16:35.1 -- not an asteroid (will add it to exclusion list)
05:49:31.76 +70:42:24.9 -- not an asteroid (will add it to exclusion list)
05:07:45.90 +67:09:35.1 -- not an asteroid (will add it to exclusion list)
04:56:44.43 +72:01:23.4 -- not an asteroid (will add it to exclusion list)
05:01:01.71 +73:12:34.2 -- not an asteroid (will add it to exclusion list)
05:33:37.30 +66:55:17.6 -- not an asteroid (will add it to exclusion list)
05:16:19.21 +70:07:06.3 -- not an asteroid (will add it to exclusion list)
05:05:52.44 +67:32:38.7 -- not an asteroid (will add it to exclusion list)
04:58:25.34 +68:15:17.1 -- not an asteroid (will add it to exclusion list)
04:49:28.13 +70:57:34.3 -- not an asteroid (will add it to exclusion list)
05:08:23.69 +65:16:32.4 -- not an asteroid (will add it to exclusion list)
04:44:44.36 +69:13:55.4 -- not an asteroid (will add it to exclusion list)
05:11:20.33 +69:34:44.2 -- not an asteroid (will add it to exclusion list)
04:33:08.27 +68:37:18.6 -- not an asteroid (will add it to exclusion list)
04:56:59.07 +74:40:32.2 -- not an asteroid (will add it to exclusion list)
04:10:55.20 +74:25:40.5 -- not an asteroid (will add it to exclusion list)
04:39:40.66 +66:13:36.1 -- not an asteroid (will add it to exclusion list)
04:51:42.42 +67:55:04.1 -- not an asteroid (will add it to exclusion list)
05:21:48.23 +66:01:58.5 -- not an asteroid (will add it to exclusion list)
05:34:31.86 +73:08:44.5 -- not an asteroid (will add it to exclusion list)
05:04:54.25 +70:09:42.7 -- not an asteroid (will add it to exclusion list)
05:30:56.00 +66:59:27.2 -- not an asteroid (will add it to exclusion list)
04:53:00.37 +71:27:22.2 -- not an asteroid (will add it to exclusion list)
05:17:28.24 +66:20:48.4 -- not an asteroid (will add it to exclusion list)
05:24:14.95 +70:32:23.3 -- not an asteroid (will add it to exclusion list)
04:35:53.98 +65:39:43.8 -- not an asteroid (will add it to exclusion list)
04:59:55.20 +69:07:50.8 -- not an asteroid (will add it to exclusion list)
04:22:18.21 +67:30:37.3 -- not an asteroid (will add it to exclusion list)
05:04:00.03 +67:32:28.1 -- not an asteroid (will add it to exclusion list)
04:37:56.89 +67:52:36.3 -- not an asteroid (will add it to exclusion list)
04:45:39.09 +66:39:26.7 -- not an asteroid (will add it to exclusion list)
04:24:21.73 +69:52:39.8 -- not an asteroid (will add it to exclusion list)
04:21:43.68 +65:21:51.4 -- not an asteroid (will add it to exclusion list)
05:10:38.40 +65:36:55.5 -- not an asteroid (will add it to exclusion list)
05:13:17.48 +66:43:01.5 -- not an asteroid (will add it to exclusion list)
04:23:46.84 +65:58:22.5 -- not an asteroid (will add it to exclusion list)
03:41:04.91 +67:38:56.4 -- not an asteroid (will add it to exclusion list)
04:05:39.68 +66:19:59.2 -- not an asteroid (will add it to exclusion list)
04:40:50.26 +68:20:36.1 -- not an asteroid (will add it to exclusion list)
05:03:01.52 +69:16:32.5 -- not an asteroid (will add it to exclusion list)
04:33:22.76 +69:56:13.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:06:41.53 +73:20:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:43.76 +72:37:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:56.28 +72:42:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:13.36 +73:06:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:36.37 +72:28:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:56.56 +72:04:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:13.68 +71:48:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:45.29 +71:39:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:17.32 +71:03:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:37.20 +71:01:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:39.36 +73:32:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:41.44 +71:22:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:02.10 +71:17:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:18.84 +71:39:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:23.56 +73:25:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:42.66 +71:26:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:43.45 +71:55:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:47.53 +72:20:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:48.96 +71:16:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:32.41 +71:22:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:37.63 +71:48:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:43.69 +73:15:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:52.33 +70:17:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:09.25 +72:27:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:35.81 +72:24:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:43.29 +70:14:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:59.00 +70:17:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:15.61 +70:14:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:22.28 +73:26:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:53.37 +73:32:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:00.40 +70:50:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:17.67 +71:01:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:36.65 +73:18:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:52.20 +69:28:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:03.49 +72:49:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:14.36 +70:37:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:15.86 +71:31:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:33.74 +71:46:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:48.71 +71:20:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:09.10 +71:46:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:31.94 +72:10:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:56.56 +70:59:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:58.99 +69:16:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:15.03 +71:53:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:35.25 +73:42:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:36.22 +69:40:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:39.83 +69:14:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:42.15 +69:26:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:46.63 +71:53:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:49.92 +73:23:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:52.60 +72:38:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:53.48 +70:34:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:12.84 +72:04:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:16.18 +72:46:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:28.85 +72:15:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:42.86 +72:17:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:54.60 +72:12:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:57.40 +68:54:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:15.19 +72:01:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:25.93 +73:51:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:44.70 +72:13:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:09.53 +73:26:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:10.52 +72:10:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:18.89 +69:58:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:20.24 +73:07:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:44.73 +69:23:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:49.82 +68:53:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:49.95 +72:24:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:57.37 +71:26:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:07.24 +70:13:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:15.39 +68:25:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:18.62 +72:38:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:25.53 +69:38:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:26.83 +70:50:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:27.13 +69:27:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:59.72 +68:07:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:16.25 +69:12:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:43.28 +68:30:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:46.42 +69:34:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:46.72 +69:49:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:49.03 +69:41:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:26:32.55 +71:04:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:26:46.00 +68:32:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:26:52.29 +67:44:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:27:23.44 +73:16:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:27:34.46 +67:15:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:05.38 +67:07:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:24.68 +67:21:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:27.76 +67:16:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:50.03 +67:18:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:58.20 +73:49:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:34.88 +67:07:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:41.33 +65:47:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:50.35 +66:06:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:08.32 +67:23:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:23.91 +65:47:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:37.84 +66:02:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:51.75 +66:55:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:06.48 +65:31:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:27.85 +65:16:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:47.13 +64:54:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:57.75 +66:13:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:03.85 +65:41:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:10.74 +65:24:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:57.98 +64:58:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:02.44 +65:09:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:04.35 +65:03:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:52.39 +64:49:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:04.83 +64:57:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:04.91 +67:38:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:11.71 +65:21:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:41.43 +70:26:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:59.86 +72:53:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:25.46 +66:01:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:56.61 +69:20:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:39.68 +66:19:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:44.65 +69:16:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:29.37 +70:10:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:53.12 +66:22:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:29.02 +66:45:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:08.78 +68:21:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:46.66 +71:04:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:47.07 +70:07:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:55.20 +74:25:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:33.52 +65:34:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:20.14 +68:01:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:07.08 +69:52:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:10.29 +69:56:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:10.34 +68:05:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:55.95 +69:09:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:01.21 +71:13:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:30.24 +65:45:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:01.18 +68:13:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:21:43.68 +65:21:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:18.21 +67:30:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:46.84 +65:58:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:07.66 +66:28:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:10.30 +70:35:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:11.86 +67:34:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:21.73 +69:52:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:34.49 +67:41:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:02.56 +66:20:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:07.72 +65:11:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:00.05 +70:46:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:19.30 +69:15:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:28.68 +69:15:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:51.41 +65:59:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:29.66 +69:08:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:07.34 +69:05:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:38.51 +65:48:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:40.13 +64:59:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:57.88 +67:16:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:08.27 +68:37:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:22.76 +69:56:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:53.77 +67:52:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:09.12 +65:02:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:49.11 +66:05:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:48.44 +65:59:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:53.98 +65:39:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:00.62 +66:19:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:51.24 +68:09:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:56.89 +67:52:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:02.78 +65:40:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:34.80 +65:24:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:00.14 +66:59:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:28.54 +68:08:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:40.66 +66:13:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:44.78 +68:25:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:25.93 +66:00:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:37.36 +66:51:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:50.26 +68:20:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:09.29 +67:50:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:43.29 +68:50:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:14.61 +69:04:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:27.97 +68:36:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:28.43 +68:14:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:43:33.40 +68:31:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:18.83 +65:11:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:44.36 +69:13:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:01.40 +66:58:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:29.01 +74:16:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:39.09 +66:39:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:55.60 +68:04:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:15.03 +66:27:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:38.69 +67:36:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:41.80 +69:27:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:00.21 +70:52:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:15.36 +71:09:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:28.13 +70:57:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:35.97 +70:19:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:39.91 +65:30:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:40.41 +66:03:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:16.55 +72:56:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:22.61 +72:53:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:08.18 +69:25:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:10.17 +67:30:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:42.42 +67:55:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:20.32 +66:13:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:47.11 +67:49:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:00.37 +71:27:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:10.49 +66:33:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:12.16 +70:21:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:36.69 +68:12:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:16.80 +65:21:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:35.41 +65:43:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:33.28 +66:54:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:09.41 +64:58:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:10.62 +65:17:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:31.70 +72:51:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.61 +66:02:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:44.43 +72:01:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:59.07 +74:40:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:11.50 +68:24:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:14.40 +69:47:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:18.04 +73:03:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:00.75 +64:59:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:07.28 +67:47:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.36 +68:55:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:25.34 +68:15:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:39.37 +66:34:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:06.11 +65:22:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:11.91 +68:56:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:42.61 +68:55:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:55.20 +69:07:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:51.56 +66:17:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:00.33 +67:24:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:01.71 +73:12:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:54.70 +71:44:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:51.25 +66:09:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:01.52 +69:16:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:25.11 +68:43:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:33.67 +65:44:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:35.97 +68:40:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:50.20 +67:50:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:55.30 +66:34:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:00.03 +67:32:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:54.25 +70:09:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:52.44 +67:32:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:57.61 +67:42:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:06.59 +65:02:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:27.05 +73:55:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:45.90 +67:09:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:54.88 +70:14:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:59.96 +65:47:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:12.10 +70:39:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:23.69 +65:16:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:36.53 +67:53:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:37.97 +67:34:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:24.68 +69:45:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:25.35 +72:12:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:38.40 +65:36:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:20.33 +69:34:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:16.01 +71:06:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:17.48 +66:43:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:37.00 +68:17:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:42.86 +74:54:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:49.52 +68:54:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:42.78 +70:06:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:43.20 +67:43:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:55.39 +73:40:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:19.21 +70:07:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:28.24 +66:20:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:42.93 +68:16:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:51.78 +68:38:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:29.74 +68:23:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:32.04 +70:53:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:24.42 +67:05:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:23.77 +66:54:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.16 +66:22:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:07.22 +73:47:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:14.70 +71:13:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:48.23 +66:01:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:14.73 +73:37:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:27.76 +69:02:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:14.41 +73:27:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:14.95 +70:32:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:27.29 +68:03:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:31.96 +73:04:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:52.22 +71:45:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:36.97 +71:07:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:08.09 +72:06:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:51.53 +70:26:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:37.95 +70:26:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:51.59 +72:20:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:09.22 +72:28:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:38.77 +74:24:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:56.00 +66:59:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:07.06 +69:18:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:38.92 +71:28:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:07.50 +73:20:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:37.30 +66:55:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:04.06 +68:50:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:31.86 +73:08:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:59.02 +70:13:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:58.51 +72:33:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:34.10 +72:33:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:48.94 +69:57:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:11.87 +69:35:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:39.98 +72:33:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:41.51 +70:56:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:44.09 +73:30:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:28.44 +64:32:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:03.79 +71:54:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:20.74 +71:28:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:27.83 +68:07:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:03.77 +70:50:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:31.76 +70:42:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:27.95 +70:32:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:24.79 +67:33:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:40.37 +71:02:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:11.41 +73:30:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:09.66 +68:03:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:29.94 +73:26:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:45.46 +69:29:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:08.07 +67:40:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:10.88 +71:30:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:53.99 +68:10:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:00.15 +70:38:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
03:06:41.53 +73:20:49.8 -- not a known variable star
03:08:43.76 +72:37:13.7 -- not a known variable star
03:08:56.28 +72:42:54.3 -- not a known variable star
03:09:13.36 +73:06:14.4 -- not a known variable star
03:09:36.37 +72:28:22.0 -- not a known variable star
03:09:56.56 +72:04:47.6 -- not a known variable star
03:11:13.68 +71:48:52.0 -- not a known variable star
03:11:45.29 +71:39:17.0 -- not a known variable star
03:12:17.32 +71:03:39.3 -- not a known variable star
03:12:37.20 +71:01:07.3 -- not a known variable star
03:12:39.36 +73:32:41.3 -- a known variable star
03:12:41.44 +71:22:37.7 -- not a known variable star
03:13:02.10 +71:17:23.4 -- not a known variable star
03:13:18.84 +71:39:25.6 -- not a known variable star
03:13:23.56 +73:25:48.0 -- not a known variable star
03:13:42.66 +71:26:02.0 -- not a known variable star
03:13:43.45 +71:55:12.5 -- not a known variable star
03:13:47.53 +72:20:15.9 -- not a known variable star
03:13:48.96 +71:16:02.0 -- not a known variable star
03:14:32.41 +71:22:49.7 -- not a known variable star
03:14:37.63 +71:48:15.1 -- not a known variable star
03:14:43.69 +73:15:53.3 -- not a known variable star
03:14:52.33 +70:17:28.3 -- not a known variable star
03:15:09.25 +72:27:59.4 -- a known variable star
03:15:35.81 +72:24:24.1 -- a known variable star
03:15:43.29 +70:14:29.2 -- not a known variable star
03:15:59.00 +70:17:15.3 -- not a known variable star
03:16:15.61 +70:14:20.2 -- a known variable star
03:16:22.28 +73:26:00.9 -- not a known variable star
03:16:53.37 +73:32:41.2 -- not a known variable star
03:17:00.40 +70:50:19.7 -- not a known variable star
03:17:17.67 +71:01:34.9 -- a known variable star
03:17:36.65 +73:18:06.8 -- a known variable star
03:17:52.20 +69:28:34.6 -- a known variable star
03:18:03.49 +72:49:34.1 -- not a known variable star
03:18:14.36 +70:37:20.7 -- not a known variable star
03:18:15.86 +71:31:05.7 -- not a known variable star
03:18:33.74 +71:46:41.9 -- not a known variable star
03:18:48.71 +71:20:47.5 -- not a known variable star
03:19:09.10 +71:46:37.1 -- not a known variable star
03:19:31.94 +72:10:47.9 -- not a known variable star
03:19:56.56 +70:59:48.9 -- not a known variable star
03:19:58.99 +69:16:23.3 -- a known variable star
03:20:15.03 +71:53:03.1 -- a known variable star
03:20:35.25 +73:42:58.0 -- not a known variable star
03:20:36.22 +69:40:29.2 -- not a known variable star
03:20:39.83 +69:14:05.7 -- not a known variable star
03:20:42.15 +69:26:29.3 -- not a known variable star
03:20:46.63 +71:53:16.4 -- a known variable star
03:20:49.92 +73:23:30.7 -- not a known variable star
03:20:52.60 +72:38:20.7 -- not a known variable star
03:20:53.48 +70:34:05.8 -- not a known variable star
03:21:12.84 +72:04:33.5 -- not a known variable star
03:21:16.18 +72:46:17.9 -- not a known variable star
03:21:28.85 +72:15:44.2 -- a known variable star
03:21:42.86 +72:17:50.9 -- not a known variable star
03:21:54.60 +72:12:50.2 -- not a known variable star
03:21:57.40 +68:54:10.0 -- not a known variable star
03:22:15.19 +72:01:37.7 -- not a known variable star
03:22:25.93 +73:51:49.3 -- not a known variable star
03:22:44.70 +72:13:06.0 -- not a known variable star
03:23:09.53 +73:26:44.5 -- not a known variable star
03:23:10.52 +72:10:59.6 -- not a known variable star
03:23:18.89 +69:58:47.0 -- not a known variable star
03:23:20.24 +73:07:29.1 -- a known variable star
03:23:44.73 +69:23:58.9 -- not a known variable star
03:23:49.82 +68:53:43.6 -- not a known variable star
03:23:49.95 +72:24:42.1 -- not a known variable star
03:23:57.37 +71:26:46.7 -- a known variable star
03:24:07.24 +70:13:44.0 -- not a known variable star
03:24:15.39 +68:25:18.5 -- not a known variable star
03:24:18.62 +72:38:27.2 -- not a known variable star
03:24:25.53 +69:38:10.4 -- not a known variable star
03:24:26.83 +70:50:47.3 -- not a known variable star
03:24:27.13 +69:27:01.7 -- not a known variable star
03:24:59.72 +68:07:51.3 -- not a known variable star
03:25:16.25 +69:12:39.7 -- not a known variable star
03:25:43.28 +68:30:54.2 -- a known variable star
03:25:46.42 +69:34:24.4 -- not a known variable star
03:25:46.72 +69:49:37.8 -- not a known variable star
03:25:49.03 +69:41:05.1 -- a known variable star
03:26:32.55 +71:04:43.6 -- not a known variable star
03:26:46.00 +68:32:03.9 -- not a known variable star
03:26:52.29 +67:44:42.9 -- not a known variable star
03:27:23.44 +73:16:40.5 -- not a known variable star
03:27:34.46 +67:15:09.2 -- not a known variable star
03:28:05.38 +67:07:18.0 -- not a known variable star
03:28:24.68 +67:21:36.8 -- not a known variable star
03:28:27.76 +67:16:28.9 -- not a known variable star
03:28:50.03 +67:18:28.0 -- not a known variable star
03:29:58.20 +73:49:29.5 -- not a known variable star
03:32:34.88 +67:07:40.9 -- a known variable star
03:32:41.33 +65:47:02.6 -- not a known variable star
03:32:50.35 +66:06:24.3 -- not a known variable star
03:33:08.32 +67:23:34.8 -- not a known variable star
03:33:23.91 +65:47:14.7 -- not a known variable star
03:34:37.84 +66:02:00.9 -- not a known variable star
03:34:51.75 +66:55:44.1 -- not a known variable star
03:35:06.48 +65:31:51.5 -- a known variable star
03:35:27.85 +65:16:45.9 -- not a known variable star
03:35:47.13 +64:54:42.0 -- not a known variable star
03:35:57.75 +66:13:34.2 -- not a known variable star
03:36:03.85 +65:41:48.0 -- not a known variable star
03:37:10.74 +65:24:41.2 -- not a known variable star
03:37:57.98 +64:58:21.5 -- not a known variable star
03:38:02.44 +65:09:10.1 -- not a known variable star
03:38:04.35 +65:03:18.0 -- not a known variable star
03:39:52.39 +64:49:08.8 -- not a known variable star
03:40:04.83 +64:57:22.5 -- not a known variable star
03:41:04.91 +67:38:56.4 -- a known variable star
03:42:11.71 +65:21:10.5 -- not a known variable star
03:59:41.43 +70:26:56.0 -- not a known variable star
03:59:59.86 +72:53:40.8 -- not a known variable star
04:02:25.46 +66:01:48.3 -- a known variable star
04:04:56.61 +69:20:11.2 -- not a known variable star
04:05:39.68 +66:19:59.2 -- a known variable star
04:05:44.65 +69:16:48.3 -- not a known variable star
04:06:29.37 +70:10:40.9 -- not a known variable star
04:06:53.12 +66:22:13.5 -- not a known variable star
04:09:29.02 +66:45:48.7 -- a known variable star
04:10:08.78 +68:21:09.3 -- not a known variable star
04:10:46.66 +71:04:07.4 -- not a known variable star
04:10:47.07 +70:07:30.0 -- not a known variable star
04:10:55.20 +74:25:40.5 -- not a known variable star
04:11:33.52 +65:34:23.1 -- not a known variable star
04:12:20.14 +68:01:10.0 -- not a known variable star
04:15:07.08 +69:52:49.4 -- not a known variable star
04:15:10.29 +69:56:54.5 -- not a known variable star
04:15:10.34 +68:05:26.0 -- not a known variable star
04:16:55.95 +69:09:50.1 -- not a known variable star
04:18:01.21 +71:13:54.8 -- a known variable star
04:18:30.24 +65:45:02.5 -- not a known variable star
04:20:01.18 +68:13:23.8 -- not a known variable star
04:21:43.68 +65:21:51.4 -- not a known variable star
04:22:18.21 +67:30:37.3 -- not a known variable star
04:23:46.84 +65:58:22.5 -- not a known variable star
04:24:07.66 +66:28:22.4 -- not a known variable star
04:24:10.30 +70:35:42.2 -- not a known variable star
04:24:11.86 +67:34:11.7 -- not a known variable star
04:24:21.73 +69:52:39.8 -- not a known variable star
04:24:34.49 +67:41:11.5 -- not a known variable star
04:26:02.56 +66:20:55.3 -- not a known variable star
04:26:07.72 +65:11:15.6 -- not a known variable star
04:28:00.05 +70:46:05.3 -- not a known variable star
04:29:19.30 +69:15:32.7 -- not a known variable star
04:29:28.68 +69:15:10.9 -- not a known variable star
04:29:51.41 +65:59:09.4 -- not a known variable star
04:30:29.66 +69:08:31.8 -- not a known variable star
04:32:07.34 +69:05:37.2 -- not a known variable star
04:32:38.51 +65:48:33.5 -- not a known variable star
04:32:40.13 +64:59:59.4 -- not a known variable star
04:32:57.88 +67:16:23.9 -- not a known variable star
04:33:08.27 +68:37:18.6 -- not a known variable star
04:33:22.76 +69:56:13.2 -- a known variable star
04:33:53.77 +67:52:43.2 -- not a known variable star
04:34:09.12 +65:02:33.6 -- not a known variable star
04:34:49.11 +66:05:18.4 -- not a known variable star
04:35:48.44 +65:59:27.1 -- a known variable star
04:35:53.98 +65:39:43.8 -- a known variable star
04:36:00.62 +66:19:30.3 -- not a known variable star
04:37:51.24 +68:09:14.6 -- not a known variable star
04:37:56.89 +67:52:36.3 -- a known variable star
04:38:02.78 +65:40:20.5 -- not a known variable star
04:38:34.80 +65:24:54.1 -- not a known variable star
04:39:00.14 +66:59:08.5 -- not a known variable star
04:39:28.54 +68:08:45.8 -- not a known variable star
04:39:40.66 +66:13:36.1 -- a known variable star
04:39:44.78 +68:25:39.5 -- not a known variable star
04:40:25.93 +66:00:12.0 -- not a known variable star
04:40:37.36 +66:51:38.7 -- a known variable star
04:40:50.26 +68:20:36.1 -- not a known variable star
04:41:09.29 +67:50:55.8 -- not a known variable star
04:41:43.29 +68:50:32.3 -- not a known variable star
04:42:14.61 +69:04:10.8 -- not a known variable star
04:42:27.97 +68:36:51.8 -- not a known variable star
04:42:28.43 +68:14:34.9 -- not a known variable star
04:43:33.40 +68:31:39.8 -- not a known variable star
04:44:18.83 +65:11:40.3 -- not a known variable star
04:44:44.36 +69:13:55.4 -- not a known variable star
04:45:01.40 +66:58:29.5 -- not a known variable star
04:45:29.01 +74:16:14.9 -- not a known variable star
04:45:39.09 +66:39:26.7 -- not a known variable star
04:45:55.60 +68:04:56.1 -- not a known variable star
04:46:15.03 +66:27:35.9 -- not a known variable star
04:46:38.69 +67:36:53.1 -- a known variable star
04:47:41.80 +69:27:47.0 -- a known variable star
04:49:00.21 +70:52:23.8 -- not a known variable star
04:49:15.36 +71:09:23.7 -- not a known variable star
04:49:28.13 +70:57:34.3 -- not a known variable star
04:49:35.97 +70:19:02.2 -- not a known variable star
04:49:39.91 +65:30:41.4 -- a known variable star
04:49:40.41 +66:03:58.7 -- not a known variable star
04:50:16.55 +72:56:16.9 -- not a known variable star
04:50:22.61 +72:53:49.7 -- not a known variable star
04:51:08.18 +69:25:23.5 -- not a known variable star
04:51:10.17 +67:30:35.6 -- not a known variable star
04:51:42.42 +67:55:04.1 -- not a known variable star
04:52:20.32 +66:13:58.9 -- not a known variable star
04:52:47.11 +67:49:23.7 -- a known variable star
04:53:00.37 +71:27:22.2 -- not a known variable star
04:53:10.49 +66:33:43.0 -- not a known variable star
04:53:12.16 +70:21:09.7 -- not a known variable star
04:53:36.69 +68:12:25.3 -- not a known variable star
04:54:16.80 +65:21:24.4 -- not a known variable star
04:54:35.41 +65:43:22.6 -- a known variable star
04:55:33.28 +66:54:53.6 -- not a known variable star
04:56:09.41 +64:58:46.4 -- not a known variable star
04:56:10.62 +65:17:00.3 -- not a known variable star
04:56:31.70 +72:51:33.2 -- not a known variable star
04:56:36.61 +66:02:19.7 -- not a known variable star
04:56:44.43 +72:01:23.4 -- not a known variable star
04:56:59.07 +74:40:32.2 -- not a known variable star
04:57:11.50 +68:24:56.5 -- not a known variable star
04:57:14.40 +69:47:59.1 -- not a known variable star
04:57:18.04 +73:03:08.3 -- not a known variable star
04:58:00.75 +64:59:19.1 -- not a known variable star
04:58:07.28 +67:47:56.5 -- not a known variable star
04:58:12.36 +68:55:42.1 -- a known variable star
04:58:25.34 +68:15:17.1 -- not a known variable star
04:58:39.37 +66:34:13.5 -- not a known variable star
04:59:06.11 +65:22:21.5 -- not a known variable star
04:59:11.91 +68:56:04.7 -- not a known variable star
04:59:42.61 +68:55:49.8 -- not a known variable star
04:59:55.20 +69:07:50.8 -- not a known variable star
05:00:51.56 +66:17:45.0 -- not a known variable star
05:01:00.33 +67:24:59.2 -- not a known variable star
05:01:01.71 +73:12:34.2 -- not a known variable star
05:01:54.70 +71:44:41.0 -- not a known variable star
05:02:51.25 +66:09:46.2 -- not a known variable star
05:03:01.52 +69:16:32.5 -- a known variable star
05:03:25.11 +68:43:25.9 -- not a known variable star
05:03:33.67 +65:44:41.9 -- not a known variable star
05:03:35.97 +68:40:11.3 -- not a known variable star
05:03:50.20 +67:50:15.1 -- not a known variable star
05:03:55.30 +66:34:55.1 -- not a known variable star
05:04:00.03 +67:32:28.1 -- not a known variable star
05:04:54.25 +70:09:42.7 -- not a known variable star
05:05:52.44 +67:32:38.7 -- a known variable star
05:05:57.61 +67:42:12.8 -- not a known variable star
05:07:06.59 +65:02:37.5 -- not a known variable star
05:07:27.05 +73:55:10.7 -- a known variable star
05:07:45.90 +67:09:35.1 -- not a known variable star
05:07:54.88 +70:14:26.2 -- not a known variable star
05:07:59.96 +65:47:23.5 -- not a known variable star
05:08:12.10 +70:39:45.2 -- not a known variable star
05:08:23.69 +65:16:32.4 -- not a known variable star
05:08:36.53 +67:53:18.6 -- not a known variable star
05:08:37.97 +67:34:29.7 -- not a known variable star
05:09:24.68 +69:45:20.8 -- not a known variable star
05:10:25.35 +72:12:14.9 -- not a known variable star
05:10:38.40 +65:36:55.5 -- not a known variable star
05:11:20.33 +69:34:44.2 -- a known variable star
05:12:16.01 +71:06:23.0 -- not a known variable star
05:13:17.48 +66:43:01.5 -- not a known variable star
05:13:37.00 +68:17:16.8 -- not a known variable star
05:14:42.86 +74:54:33.0 -- not a known variable star
05:14:49.52 +68:54:52.3 -- not a known variable star
05:15:42.78 +70:06:35.3 -- not a known variable star
05:15:43.20 +67:43:19.8 -- a known variable star
05:15:55.39 +73:40:00.6 -- not a known variable star
05:16:19.21 +70:07:06.3 -- not a known variable star
05:17:28.24 +66:20:48.4 -- not a known variable star
05:17:42.93 +68:16:35.1 -- not a known variable star
05:17:51.78 +68:38:01.5 -- not a known variable star
05:18:29.74 +68:23:54.5 -- not a known variable star
05:18:32.04 +70:53:23.7 -- not a known variable star
05:19:24.42 +67:05:13.2 -- not a known variable star
05:20:23.77 +66:54:07.5 -- a known variable star
05:20:36.16 +66:22:27.7 -- not a known variable star
05:21:07.22 +73:47:45.2 -- a known variable star
05:21:14.70 +71:13:30.4 -- not a known variable star
05:21:48.23 +66:01:58.5 -- not a known variable star
05:23:14.73 +73:37:18.3 -- not a known variable star
05:23:27.76 +69:02:17.2 -- not a known variable star
05:24:14.41 +73:27:32.5 -- not a known variable star
05:24:14.95 +70:32:23.3 -- not a known variable star
05:25:27.29 +68:03:13.0 -- not a known variable star
05:25:31.96 +73:04:27.6 -- not a known variable star
05:25:52.22 +71:45:50.9 -- not a known variable star
05:26:36.97 +71:07:51.0 -- not a known variable star
05:27:08.09 +72:06:04.5 -- not a known variable star
05:28:51.53 +70:26:47.6 -- not a known variable star
05:29:37.95 +70:26:14.1 -- not a known variable star
05:29:51.59 +72:20:59.2 -- not a known variable star
05:30:09.22 +72:28:21.0 -- not a known variable star
05:30:38.77 +74:24:25.9 -- not a known variable star
05:30:56.00 +66:59:27.2 -- not a known variable star
05:32:07.06 +69:18:10.7 -- not a known variable star
05:32:38.92 +71:28:26.7 -- not a known variable star
05:33:07.50 +73:20:44.2 -- not a known variable star
05:33:37.30 +66:55:17.6 -- not a known variable star
05:34:04.06 +68:50:00.1 -- not a known variable star
05:34:31.86 +73:08:44.5 -- not a known variable star
05:35:59.02 +70:13:11.9 -- not a known variable star
05:37:58.51 +72:33:47.4 -- not a known variable star
05:38:34.10 +72:33:43.1 -- not a known variable star
05:39:48.94 +69:57:50.5 -- a known variable star
05:40:11.87 +69:35:20.3 -- not a known variable star
05:40:39.98 +72:33:22.0 -- not a known variable star
05:41:41.51 +70:56:51.3 -- not a known variable star
05:42:44.09 +73:30:38.5 -- not a known variable star
05:44:28.44 +64:32:51.6 -- not a known variable star
05:46:03.79 +71:54:41.3 -- not a known variable star
05:46:20.74 +71:28:22.1 -- not a known variable star
05:46:27.83 +68:07:42.4 -- not a known variable star
05:49:03.77 +70:50:50.0 -- not a known variable star
05:49:31.76 +70:42:24.9 -- not a known variable star
05:52:27.95 +70:32:03.4 -- not a known variable star
05:54:24.79 +67:33:38.3 -- not a known variable star
05:54:40.37 +71:02:25.3 -- not a known variable star
05:58:11.41 +73:30:51.0 -- not a known variable star
06:00:09.66 +68:03:11.5 -- not a known variable star
06:02:29.94 +73:26:04.8 -- not a known variable star
06:03:45.46 +69:29:32.8 -- not a known variable star
06:05:08.07 +67:40:13.1 -- not a known variable star
06:07:10.88 +71:30:10.1 -- not a known variable star
06:09:53.99 +68:10:40.9 -- not a known variable star
06:15:00.15 +70:38:30.3 -- not a known variable star
Found 276 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
318 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.76158431 -observatory 500
23:23:37.29 -01:56:06.8 Mercury (-0.1mag)
23:04:53.94 -07:27:04.3 Venus (-3.9mag)
21:43:06.05 -14:51:23.4 Mars (1.1mag)
07:06:04.69 +22:54:22.5 Jupiter (-2.5mag)
00:05:28.55 -01:44:12.2 Saturn (1.0mag)
03:39:59.86 +19:21:45.0 Uranus (5.7mag)
00:03:41.60 -01:01:32.7 Neptune (7.8mag)
20:29:07.74 -22:59:32.6 Pluto (14.5mag)
01:59:17.65 +16:46:44.5 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 03:32 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461093.76158431:
07:06:11.24 +22:54:11.5 Io (5.4mag)
07:06:17.45 +22:53:58.3 Europa (5.5mag)
07:05:57.51 +22:54:44.5 Ganymede (4.9mag)
07:06:25.12 +22:53:54.2 Callisto (6.2mag)
07:09:14.09 +23:10:42.7 Himalia (15.0mag)
07:06:08.56 +22:54:15.8 Thebe (15.9mag)
07:08:39.09 +23:19:14.9 Elara (17.0mag)
07:01:38.54 +24:02:17.7 Pasiphae (17.0mag)
07:15:05.57 +22:42:24.3 Carme (18.1mag)
00:05:40.34 -01:44:16.5 Titan (8.8mag)
00:05:34.22 -01:44:10.5 Rhea (10.1mag)
00:05:24.20 -01:45:32.5 Iapetus (11.5mag)
00:05:29.77 -01:44:15.6 Hyperion (14.8mag)
00:07:32.81 -01:31:12.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 03:32 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.76158431:
08:46:36.94 +24:30:48.4 JWST
13:31:27.54 +54:14:10.1 Chandra
16:34:36.49 -51:12:46.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 03:32 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.76158431 at 500
16:59:54.05 -11:03:54.2 17.5mag 10P/Tempel 2
03:37:24.95 +28:58:11.7 18.0mag 123P/West-Hartley
08:23:28.67 +60:40:57.2 18.4mag 124P/Mrkos
21:19:55.90 -07:36:59.7 22.1mag 141P/Machholz
01:21:23.19 +11:56:39.7 17.7mag 145P/Shoemaker-Levy 5
11:02:52.90 +30:35:15.5 17.9mag 164P/Christensen
09:33:04.39 -33:51:31.1 18.0mag 195P/Hill
15:52:02.54 -06:35:16.3 19.2mag 210P/Christensen
18:17:21.31 -21:28:08.3 17.3mag 218P/LINEAR
04:45:22.04 +19:21:15.2 0.0mag 235P/LINEAR
03:56:32.55 +27:45:41.3 17.8mag 240P/NEAT
15:17:45.39 +06:37:56.2 14.8mag 24P/Schaumasse
11:23:28.47 -03:22:59.7 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.06 +27:24:52.1 19.6mag 407P/PanSTARRS-Fuls
17:07:19.41 -11:19:11.2 17.6mag 40P/Vaisala 1
11:02:08.68 -08:51:31.1 16.6mag 43P/Wolf-Harrington
13:25:30.12 -05:49:59.6 20.0mag 489P/Denning
04:34:26.93 +48:34:02.4 17.8mag 493P/2024 Q2 (LONEOS)
06:04:25.74 +47:30:16.0 17.7mag 63P/Wild 1
23:14:49.34 -02:06:19.9 16.2mag 78P/Gehrels 2
20:01:54.43 -22:17:21.6 14.9mag 88P/Howell
15:27:57.88 -29:01:11.7 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.74 -72:35:32.0 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:49.04 +31:12:55.2 18.2mag C/2017 K2 (PanSTARRS)
20:06:41.84 -65:11:50.3 18.1mag C/2020 V2 (ZTF)
17:21:43.14 +04:22:03.7 16.3mag C/2021 G2 (ATLAS)
03:35:46.20 +24:36:50.1 15.8mag C/2022 N2 (PanSTARRS)
09:08:11.01 +29:50:06.0 15.3mag C/2022 QE78 (ATLAS)
08:35:38.59 -06:32:59.0 16.7mag C/2022 R6 (PanSTARRS)
23:53:10.34 +48:27:01.5 18.0mag C/2023 C2 (ATLAS)
09:51:00.66 -20:45:02.3 17.5mag C/2023 F3 (ATLAS)
20:34:58.31 +61:14:31.3 17.3mag C/2023 H5 (Lemmon)
19:34:30.89 -03:24:19.1 16.1mag C/2023 R1 (PANSTARRS)
02:48:57.49 +35:40:31.2 18.5mag C/2023 RS61 (PanSTARRS)
21:01:37.97 +81:20:04.8 18.0mag C/2023 X2 (Lemmon)
06:39:00.28 +63:49:22.4 17.3mag C/2024 A1 (ATLAS)
01:57:33.17 -24:28:51.6 11.2mag C/2024 E1 (Wierzchos)
11:44:53.54 -02:33:36.8 18.1mag C/2024 G2 (ATLAS)
19:28:25.25 +00:39:25.8 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.53 -01:42:01.7 17.7mag C/2024 G6 (ATLAS)
19:53:32.09 +03:16:18.8 15.6mag C/2024 J3 (ATLAS)
02:47:18.07 -31:33:14.6 15.4mag C/2024 T5 (ATLAS)
16:24:48.18 -58:16:20.6 15.6mag C/2025 A6 (Lemmon)
04:50:28.23 +62:11:55.5 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:38.89 -12:55:50.7 14.8mag C/2025 L1 (ATLAS)
02:20:19.66 -19:06:53.2 16.7mag C/2025 Q3 (ATLAS)
02:09:42.86 +17:17:21.4 21.2mag C/2025 R2 (SWAN)
22:20:48.22 +17:39:24.1 16.4mag C/2025 R3 (PANSTARRS)
21:46:08.20 -16:51:48.6 21.5mag C/2025 T1 (ATLAS)
03:05:59.45 -20:30:51.4 18.3mag C/2026 A1 (MAPS)
21:03:26.47 +20:58:35.3 16.9mag C/2026 B2 (Sun-Gao)
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
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