This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J033914.97+651304.2,2461083.9979,9.72,0.05,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
ASASSN-V J033914.97+651304.2 20260212.4979 9.72CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:14.87 +65:13:13.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.36 03:54:14.31 +65:06:44.3
140.67426 8.74588 galactic Cam Second-epoch detections are separated by 1.1" and 4.7 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 489769281274844416 | 03:54:13.43 +65:06:37.8 (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 489769281274844416,2461083.9979,10.36,0.05,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 489769281274844416 20260212.4979 10.36CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:14.31 +65:06:44.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.63 03:35:50.78 +65:16:35.6
139.03953 7.68339 galactic Cam Second-epoch detections are separated by 0.8" and 4.6 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 488486804040381568 | 03:35:49.76 +65:16:32.5 (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 488486804040381568,2461083.9979,10.63,0.05,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 488486804040381568 20260212.4979 10.63CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:50.78 +65:16:35.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 15 00.22 +70 30 11.4 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 541533498435287168,2461083.9979,11.18,0.05,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
Gaia DR3 541533498435287168 20260212.4979 11.18CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:00.22 +70:30:11.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.18 03:36:12.01 +65:29:18.6
138.94310 7.87613 galactic Cam Second-epoch detections are separated by 0.2" and 4.8 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 491493281148449408 | 03:36:11.05 +65:29:14.9 (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 491493281148449408,2461083.9979,11.18,0.05,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
Gaia DR3 491493281148449408 20260212.4979 11.18CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:12.01 +65:29:18.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.36 03:13:42.44 +71:37:45.0
133.72603 11.80506 galactic Cas Second-epoch detections are separated by 3.1" and 4.9 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 543891847796964864 | 03:13:44.41 +71:37:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+71 108
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 12.4979* 03 13 42.44 +71 37 45.0 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 543891847796964864,2461083.9979,11.36,0.05,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 543891847796964864 20260212.4979 11.36CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:42.44 +71:37:45.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.47 03:44:54.11 +65:03:16.0
139.93997 8.08057 galactic Cam Second-epoch detections are separated by 0.9" and 4.6 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 488316620256579840 | 03:44:52.97 +65:03:20.2 (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 488316620256579840,2461083.9979,11.47,0.05,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 488316620256579840 20260212.4979 11.47CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:54.11 +65:03:16.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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
PW Cam,2461083.9979,11.62,0.05,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
PW Cam 20260212.4979 11.62CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:25.35 +65:16:19.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 J0356573+703428,2461083.9979,11.51,0.05,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
NSVS J0356573+703428 20260212.4979 11.51CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:58.17 +70:34:27.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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
GI Cam,2461083.9979,11.49,0.05,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
GI Cam 20260212.4979 11.49CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:03.98 +68:35:28.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 477099162111176320,2461083.9979,12.23,0.05,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 477099162111176320 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:14.46 +65:36:03.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.14 03:35:25.28 +67:46:27.5
137.51100 9.67276 galactic Cam Second-epoch detections are separated by 2.5" and 4.0 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 492014857676132480 | 03:35:25.96 +67:46:34.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 492014857676132480,2461083.9979,12.14,0.05,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 492014857676132480 20260212.4979 12.14CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:25.28 +67:46:27.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 19 57.13 +73 32 31.8 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,2461083.9979,12.38,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:57.13 +73:32:31.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.15 04:22:39.89 +68:29:26.3
140.38370 13.11861 galactic Cam Second-epoch detections are separated by 3.1" and 4.7 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 | 04:22:39.89 +68:29:26.3 (user input) | T | P | (position from user input) J-Ks=1.324+/- (Very red! L if it's a dwarf)
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,2461083.9979,12.15,0.05,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
target 20260212.4979 12.15CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:39.89 +68:29:26.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.95 03:41:15.95 +66:16:44.3
138.88231 8.81895 galactic Cam Second-epoch detections are separated by 3.3" and 5.0 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 491637312871393664 | 03:41:16.86 +66:16:40.7 (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 491637312871393664,2461083.9979,11.95,0.05,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 491637312871393664 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:15.95 +66:16:44.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,11.96,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:51.63 +65:54:40.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.96 03:28:48.37 +69:27:28.7
136.01577 10.68862 galactic Cas Second-epoch detections are separated by 3.4" and 4.7 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 494648570280662144 | 03:28:49.61 +69:27:26.5 (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 12.4979* 03 28 48.37 +69 27 28.7 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
Gaia DR3 494648570280662144,2461083.9979,11.96,0.05,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
Gaia DR3 494648570280662144 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:48.37 +69:27:28.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.74 03:22:29.99 +70:00:50.4
135.23749 10.83921 galactic Cas Second-epoch detections are separated by 8.4" and 5.8 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 542760312893443200 | 03:22:29.73 +70:01:08.3 (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 12.4979* 03 22 29.99 +70 00 50.4 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 542760312893443200,2461083.9979,11.74,0.05,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 542760312893443200 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:29.99 +70:00:50.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.78 03:23:14.61 +70:01:35.0
135.28424 10.88484 galactic Cas Second-epoch detections are separated by 2.8" and 4.5 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 542760931365833344 | 03:23:15.20 +70:01:17.2 (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 12.4979* 03 23 14.61 +70 01 35.0 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 542760931365833344,2461083.9979,11.78,0.05,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 542760931365833344 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:14.61 +70:01:35.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 642397,2461083.9979,11.81,0.05,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
NSVS 642397 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:01.24 +68:13:19.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.50 03:32:19.85 +67:40:17.6
137.33185 9.41756 galactic Cam Second-epoch detections are separated by 1.6" and 4.7 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 492758681591812352 | 03:32:21.35 +67:40:22.7 (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 492758681591812352,2461083.9979,11.50,0.05,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
Gaia DR3 492758681591812352 20260212.4979 11.50CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:19.85 +67:40:17.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.27 03:43:00.94 +66:17:03.1
139.02013 8.93053 galactic Cam Second-epoch detections are separated by 7.8" and 4.6 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 491634430949529088 | 03:43:01.99 +66:17:04.2 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 491634430949529088,2461083.9979,11.27,0.05,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
Gaia DR3 491634430949529088 20260212.4979 11.27CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:00.94 +66:17:03.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.99 05:10:02.21 +68:35:20.7
143.06610 16.58342 galactic Cam Second-epoch detections are separated by 1.0" and 4.3 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 483854144937258368 | 05:10:02.22 +68:35:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.245+/-0.035 (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 483854144937258368,2461083.9979,10.99,0.05,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
Gaia DR3 483854144937258368 20260212.4979 10.99CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:02.21 +68:35:20.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 9.31 03:42:25.66 +64:48:24.0
139.88446 7.72412 galactic Cam Second-epoch detections are separated by 0.6" and 4.7 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 488216324179547008 | 03:42:25.90 +64:48:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+64 239
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 488216324179547008,2461083.9979,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 488216324179547008 20260212.4979 9.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:25.66 +64:48:24.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 9.66 03:19:32.15 +69:24:55.3
135.35395 10.19793 galactic Cas Second-epoch detections are separated by 2.9" and 4.1 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 541194230378557952 | 03:19:33.73 +69:24:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+69 150
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 12.4979* 03 19 32.15 +69 24 55.3 9.7 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 541194230378557952,2461083.9979,9.66,0.05,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 541194230378557952 20260212.4979 9.66CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:32.15 +69:24:55.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 9.86 03:12:46.84 +73:28:15.2
132.66761 13.33136 galactic Cas Second-epoch detections are separated by 6.0" and 4.3 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 544359896152218240 | 03:12:48.43 +73:28:16.9 (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 12.4979* 03 12 46.84 +73 28 15.2 9.9 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 544359896152218240,2461083.9979,9.86,0.05,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 544359896152218240 20260212.4979 9.86CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:46.84 +73:28:15.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 9.71 03:43:46.25 +65:17:29.2
139.69806 8.19422 galactic Cam Second-epoch detections are separated by 6.9" and 4.8 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 488513261038803840 | 03:43:47.29 +65:17:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+65 227
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 488513261038803840,2461083.9979,9.71,0.05,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 488513261038803840 20260212.4979 9.71CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:46.25 +65:17:29.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 9.97 03:13:37.14 +70:50:51.2
134.14105 11.13757 galactic Cas Second-epoch detections are separated by 0.9" and 4.6 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 541557378453245696 | 03:13:40.87 +70:50:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956PMcCO..13a....B AG+70 162
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 12.4979* 03 13 37.14 +70 50 51.2 10.0 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 541557378453245696,2461083.9979,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 541557378453245696 20260212.4979 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:37.14 +70:50:51.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.03 03:24:41.48 +68:45:11.8
136.11485 9.90017 galactic Cas Second-epoch detections are separated by 2.5" and 4.0 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 493110216074945664 | 03:24:43.57 +68:45:13.0 (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 12.4979* 03 24 41.48 +68 45 11.8 10.0 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 493110216074945664,2461083.9979,10.03,0.05,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
Gaia DR3 493110216074945664 20260212.4979 10.03CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:41.48 +68:45:11.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.35 03:23:08.24 +69:38:53.2
135.49091 10.56556 galactic Cas Second-epoch detections are separated by 0.9" and 4.5 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 541201033606972672 | 03:23:09.95 +69:38:53.4 (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 12.4979* 03 23 08.24 +69 38 53.2 10.3 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 541201033606972672,2461083.9979,10.35,0.05,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 541201033606972672 20260212.4979 10.35CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:08.24 +69:38:53.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.49 03:13:11.66 +72:36:29.3
133.16214 12.61512 galactic Cas Second-epoch detections are separated by 1.9" and 4.6 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 544249567033278592 | 03:13:13.18 +72:36:30.8 (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 12.4979* 03 13 11.66 +72 36 29.3 10.5 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 544249567033278592,2461083.9979,10.49,0.05,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 544249567033278592 20260212.4979 10.49CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:11.66 +72:36:29.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.68 03:17:43.97 +72:32:06.5
133.49627 12.73574 galactic Cas Second-epoch detections are separated by 8.4" and 4.7 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 544051929817573888 | 03:17:45.58 +72:32:03.6 (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 12.4979* 03 17 43.97 +72 32 06.5 10.7 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 544051929817573888,2461083.9979,10.68,0.05,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 544051929817573888 20260212.4979 10.68CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:43.97 +72:32:06.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.51 03:22:54.84 +68:33:48.0
136.08597 9.65234 galactic Cas Second-epoch detections are separated by 5.8" and 3.8 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 493083724716796288 | 03:22:56.64 +68:33:50.5 (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 12.4979* 03 22 54.84 +68 33 48.0 10.5 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 493083724716796288,2461083.9979,10.51,0.05,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
Gaia DR3 493083724716796288 20260212.4979 10.51CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:54.84 +68:33:48.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.61 03:19:43.93 +69:27:22.1
135.34606 10.24152 galactic Cas Second-epoch detections are separated by 1.7" and 4.2 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 541194432239367936 | 03:19:45.99 +69:27:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1956PMcCO..13a....B AG+69 151
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 12.4979* 03 19 43.93 +69 27 22.1 10.6 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 541194432239367936,2461083.9979,10.61,0.05,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 541194432239367936 20260212.4979 10.61CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:43.93 +69:27:22.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.67 03:21:05.38 +70:35:23.4
134.81210 11.25321 galactic Cas Second-epoch detections are separated by 1.1" and 4.3 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 542980455737217408 | 03:21:07.51 +70:35:24.9 (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 12.4979* 03 21 05.38 +70 35 23.4 10.7 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 542980455737217408,2461083.9979,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 542980455737217408 20260212.4979 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:05.38 +70:35:23.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.68 03:18:31.95 +71:59:23.6
133.85272 12.31158 galactic Cas Second-epoch detections are separated by 5.5" and 4.3 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 543879718810226048 | 03:18:34.67 +71:59:20.5 (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 12.4979* 03 18 31.95 +71 59 23.6 10.7 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 543879718810226048,2461083.9979,10.68,0.05,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 543879718810226048 20260212.4979 10.68CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:31.95 +71:59:23.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.61 03:27:41.45 +67:32:24.1
137.04228 9.05575 galactic Cam Second-epoch detections are separated by 3.5" and 4.0 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 492744525379364864 | 03:27:44.25 +67:32:29.6 (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 492744525379364864,2461083.9979,10.61,0.05,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 492744525379364864 20260212.4979 10.61CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:41.45 +67:32:24.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.59 03:38:54.28 +65:23:50.6
139.22576 7.97036 galactic Cam Second-epoch detections are separated by 1.3" and 4.6 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 488481272122416640 | 03:38:53.37 +65:23:48.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 488481272122416640,2461083.9979,10.59,0.05,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 488481272122416640 20260212.4979 10.59CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:54.28 +65:23:50.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.94 03:11:44.36 +71:39:22.9
133.57678 11.74675 galactic Cas Second-epoch detections are separated by 3.8" and 4.5 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 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 12.4979* 03 11 44.36 +71 39 22.9 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 543894115539708672,2461083.9979,10.94,0.05,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 543894115539708672 20260212.4979 10.94CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:44.36 +71:39:22.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.01 03:11:35.67 +71:41:32.4
133.54767 11.77148 galactic Cas Second-epoch detections are separated by 1.9" and 4.7 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 543895180691347968 | 03:11:37.67 +71:41:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.685+/-0.410 (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!
TCP 2026 02 12.4979* 03 11 35.67 +71 41 32.4 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
Gaia DR3 543895180691347968,2461083.9979,11.01,0.05,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
Gaia DR3 543895180691347968 20260212.4979 11.01CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:35.67 +71:41:32.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.01 05:02:20.34 +72:25:34.8
139.33661 18.15338 galactic Cam Second-epoch detections are separated by 0.6" and 4.3 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 499149902163929472 | 05:02:17.51 +72:25:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.026 (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 499149902163929472,2461083.9979,11.01,0.05,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
Gaia DR3 499149902163929472 20260212.4979 11.01CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:20.34 +72:25:34.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.13 03:11:12.76 +71:36:40.6
133.56463 11.68664 galactic Cas Second-epoch detections are separated by 4.2" and 4.4 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 543894321699020160 | 03:11:15.11 +71:36:39.2 (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 12.4979* 03 11 12.76 +71 36 40.6 11.1 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 543894321699020160,2461083.9979,11.13,0.05,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 543894321699020160 20260212.4979 11.13CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:12.76 +71:36:40.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 488440865071737472,2461083.9979,10.91,0.05,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 488440865071737472 20260212.4979 10.91CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:18.86 +64:54:29.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 488440865071737472,2461083.9979,10.88,0.05,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 488440865071737472 20260212.4979 10.88CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:16.45 +64:54:22.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 10.99 04:51:34.01 +68:12:02.3
142.38342 14.96836 galactic Cam Second-epoch detections are separated by 0.8" and 4.1 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 | 04:51:34.01 +68:12:02.3 (user input) | T | P | (position from user input) J-Ks=0.693+/-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,2461083.9979,10.99,0.05,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 20260212.4979 10.99CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:34.01 +68:12:02.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.30 04:42:14.55 +69:04:10.5
141.13405 14.83358 galactic Cam Second-epoch detections are separated by 0.8" and 4.3 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 | 04:42:14.55 +69:04:10.5 (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,2461083.9979,11.30,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:14.55 +69:04:10.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.31 03:11:06.49 +72:08:33.3
133.27475 12.13597 galactic Cas Second-epoch detections are separated by 8.6" and 5.0 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 544128070998630272 | 03:11:08.00 +72:08:34.1 (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 12.4979* 03 11 06.49 +72 08 33.3 11.3 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 544128070998630272,2461083.9979,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 544128070998630272 20260212.4979 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:06.49 +72:08:33.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.43 04:51:32.82 +68:11:46.1
142.38599 14.96417 galactic Cam Second-epoch detections are separated by 1.9" and 4.1 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 | 04:51:32.82 +68:11:46.1 (user input) | T | P | (position from user input) J-Ks=0.277+/-0.030 (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,2461083.9979,11.43,0.05,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 20260212.4979 11.43CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:32.82 +68:11:46.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.24 03:17:24.50 +71:45:17.0
133.90833 12.06664 galactic Cas Second-epoch detections are separated by 7.7" and 4.6 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 543872709422612224 | 03:17:26.31 +71:45:14.8 (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 12.4979* 03 17 24.50 +71 45 17.0 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 543872709422612224,2461083.9979,11.24,0.05,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 543872709422612224 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:24.50 +71:45:17.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.43 05:13:54.01 +67:29:16.7
144.23580 16.29326 galactic Cam Second-epoch detections are separated by 0.9" and 4.2 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 | 05:13:54.01 +67:29:16.7 (user input) | T | P | (position from user input) J-Ks=0.817+/-0.030 (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,2461083.9979,11.43,0.05,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 20260212.4979 11.43CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:54.01 +67:29:16.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.60 04:18:40.76 +74:39:10.7
135.50255 17.10310 galactic Cam Second-epoch detections are separated by 0.4" and 4.4 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 | 04:18:40.76 +74:39:10.7 (user input) | T | P | (position from user input) J-Ks=0.544+/-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,2461083.9979,11.60,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:40.76 +74:39:10.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.59 03:14:16.07 +70:32:08.8
134.35521 10.90115 galactic Cas Second-epoch detections are separated by 8.1" and 4.8 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 541537140567553536 | 03:14:17.29 +70:32:10.2 (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 12.4979* 03 14 16.07 +70 32 08.8 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 541537140567553536,2461083.9979,11.59,0.05,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 541537140567553536 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:16.07 +70:32:08.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.32 03:30:00.25 +67:45:04.3
137.10281 9.35475 galactic Cam Second-epoch detections are separated by 4.6" and 3.8 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 492751947083100288 | 03:30:02.62 +67:45:05.5 (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 492751947083100288,2461083.9979,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 492751947083100288 20260212.4979 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:00.25 +67:45:04.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.36 03:35:27.04 +65:32:13.9
138.85079 7.86956 galactic Cam Second-epoch detections are separated by 0.5" and 4.8 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 491494277579582592 | 03:35:25.92 +65:32:08.5 (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 491494277579582592,2461083.9979,11.36,0.05,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 491494277579582592 20260212.4979 11.36CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:27.04 +65:32:13.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.54 03:19:36.54 +72:06:51.2
133.85414 12.46102 galactic Cas Second-epoch detections are separated by 8.2" and 4.4 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 543976059217920128 | 03:19:38.45 +72:06:54.6 (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 12.4979* 03 19 36.54 +72 06 51.2 11.5 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 543976059217920128,2461083.9979,11.54,0.05,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 543976059217920128 20260212.4979 11.54CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:36.54 +72:06:51.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.56 03:16:06.92 +72:04:22.5
133.64630 12.28044 galactic Cas Second-epoch detections are separated by 2.8" and 4.7 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 543931700795982080 | 03:16:09.46 +72:04:21.1 (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 12.4979* 03 16 06.92 +72 04 22.5 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 543931700795982080,2461083.9979,11.56,0.05,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
Gaia DR3 543931700795982080 20260212.4979 11.56CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:06.92 +72:04:22.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.65 04:57:37.86 +70:38:34.7
140.65844 16.83815 galactic Cam Second-epoch detections are separated by 0.9" and 4.2 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 | 04:57:37.86 +70:38:34.7 (user input) | T | P | (position from user input) J-Ks=0.643+/-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,2461083.9979,11.65,0.05,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 20260212.4979 11.65CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:37.86 +70:38:34.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.45 03:38:42.01 +65:20:21.7
139.24366 7.91114 galactic Cam Second-epoch detections are separated by 2.0" and 5.1 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 488478798221271168 | 03:38:40.97 +65:20:18.5 (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 488478798221271168,2461083.9979,11.45,0.05,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 488478798221271168 20260212.4979 11.45CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:42.01 +65:20:21.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.62 03:16:27.35 +72:23:52.9
133.48948 12.56840 galactic Cas Second-epoch detections are separated by 2.0" and 4.1 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 544043713542750720 | 03:16:29.46 +72:23:52.6 (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 12.4979* 03 16 27.35 +72 23 52.9 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 544043713542750720,2461083.9979,11.62,0.05,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 544043713542750720 20260212.4979 11.62CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:27.35 +72:23:52.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 07 46.27 +72 53 43.2 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 544224931100531584,2461083.9979,11.79,0.05,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 544224931100531584 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:46.27 +72:53:43.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.74 04:02:57.94 +72:49:32.9
136.04008 15.03487 galactic Cam Second-epoch detections are separated by 0.8" and 4.3 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 | 04:02:57.94 +72:49:32.9 (user input) | T | P | (position from user input) J-Ks=0.639+/-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,2461083.9979,11.74,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:57.94 +72:49:32.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.54 03:35:20.92 +65:32:13.2
138.84230 7.86318 galactic Cam Second-epoch detections are separated by 4.3" and 4.7 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 491494277579582592 | 03:35:25.92 +65:32:08.5 (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 491494277579582592,2461083.9979,11.54,0.05,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 491494277579582592 20260212.4979 11.54CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:20.92 +65:32:13.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.84 05:20:28.75 +71:45:06.8
140.71455 18.98546 galactic Cam Second-epoch detections are separated by 0.3" and 4.1 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 498168141359879040 | 05:20:35.62 +71:44:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.465+/-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 498168141359879040,2461083.9979,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 498168141359879040 20260212.4979 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:28.75 +71:45:06.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.73 03:25:28.24 +67:58:18.1
136.61970 9.29334 galactic Cam Second-epoch detections are separated by 2.6" and 5.0 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 492816612110369536 | 03:25:30.35 +67:58:20.9 (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 492816612110369536,2461083.9979,11.73,0.05,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 492816612110369536 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:28.24 +67:58:18.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.55 03:41:10.31 +65:18:53.6
139.46638 8.04710 galactic Cam Second-epoch detections are separated by 2.5" and 4.9 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 J055.2820+65.3105 | 03:41:08.87 +65:18:50.3 (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 J055.2820+65.3105,2461083.9979,11.55,0.05,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
ATO J055.2820+65.3105 20260212.4979 11.55CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:10.31 +65:18:53.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.64 03:39:47.90 +64:48:07.8
139.66255 7.55104 galactic Cam Second-epoch detections are separated by 6.2" and 4.8 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 488398087196420736 | 03:39:47.34 +64:48:12.6 (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 488398087196420736,2461083.9979,11.64,0.05,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 488398087196420736 20260212.4979 11.64CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:47.90 +64:48:07.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.71 03:35:48.57 +64:54:50.6
139.25215 7.38845 galactic Cam Second-epoch detections are separated by 5.4" and 5.4 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 488440143517235712 | 03:35:47.66 +64:54:49.2 (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 488440143517235712,2461083.9979,11.71,0.05,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 488440143517235712 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:48.57 +64:54:50.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.70 03:08:43.30 +72:37:12.3
132.86370 12.45111 galactic Cas Second-epoch detections are separated by 3.4" and 4.7 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 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 12.4979* 03 08 43.30 +72 37 12.3 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 544200737547278464,2461083.9979,11.70,0.05,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
Gaia DR3 544200737547278464 20260212.4979 11.70CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:43.30 +72:37:12.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.86 05:58:41.51 +66:36:24.1
147.18255 19.74855 galactic Cam Second-epoch detections are separated by 1.5" and 4.0 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 480401923239948928 | 05:58:44.68 +66:36:07.8 (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) J-Ks=0.337+/-0.030 (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 480401923239948928,2461083.9979,11.86,0.05,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
Large-amplitude variable Gaia DR2 480401923239948928 20260212.4979 11.86CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:41.51 +66:36:24.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 22 50.05 +73 24 19.5 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
Gaia DR3 544673871146138752,2461083.9979,11.99,0.05,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
Gaia DR3 544673871146138752 20260212.4979 11.99CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:50.05 +73:24:19.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.92 04:47:21.97 +70:17:06.1
140.42895 15.93489 galactic Cam Second-epoch detections are separated by 0.2" and 4.3 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 | 04:47:21.97 +70:17:06.1 (user input) | T | P | (position from user input) J-Ks=0.430+/-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,2461083.9979,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:21.97 +70:17:06.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.84 05:14:25.32 +69:50:42.1
142.17303 17.58335 galactic Cam Second-epoch detections are separated by 1.9" and 4.4 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 | 05:14:25.32 +69:50:42.1 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.030 (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,2461083.9979,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:25.32 +69:50:42.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.05 03:11:51.22 +73:33:27.1
132.56321 13.37027 galactic Cas Second-epoch detections are separated by 5.8" and 4.4 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 547363757623605248 | 03:11:52.89 +73:33:30.7 (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 12.4979* 03 11 51.22 +73 33 27.1 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 547363757623605248,2461083.9979,12.05,0.05,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 547363757623605248 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:51.22 +73:33:27.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 10 17.27 +72 32 36.5 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
Gaia DR3 544157586013399168,2461083.9979,11.96,0.05,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
Gaia DR3 544157586013399168 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:17.27 +72:32:36.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.82 03:15:50.18 +73:22:59.9
132.90502 13.37367 galactic Cas Second-epoch detections are separated by 7.2" and 5.2 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 544344502989574272 | 03:15:51.39 +73:23:02.7 (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 12.4979* 03 15 50.18 +73 22 59.9 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 544344502989574272,2461083.9979,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 544344502989574272 20260212.4979 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:50.18 +73:22:59.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.86 03:35:46.07 +64:54:43.9
139.24967 7.38435 galactic Cam Second-epoch detections are separated by 0.6" and 4.6 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 488440143517235712 | 03:35:47.66 +64:54:49.2 (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 488440143517235712,2461083.9979,11.86,0.05,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 488440143517235712 20260212.4979 11.86CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:46.07 +64:54:43.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.77 03:27:15.02 +67:49:32.8
136.84316 9.26731 galactic Cam Second-epoch detections are separated by 8.3" and 3.9 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 492799569680160768 | 03:27:16.73 +67:49:39.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 492799569680160768,2461083.9979,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 492799569680160768 20260212.4979 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:15.02 +67:49:32.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.79 03:34:48.29 +65:06:05.0
139.05446 7.47748 galactic Cam Second-epoch detections are separated by 2.0" and 4.9 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 488457735701811200 | 03:34:47.41 +65:06:02.3 (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 488457735701811200,2461083.9979,11.79,0.05,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 488457735701811200 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:48.29 +65:06:05.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.82 03:37:59.67 +64:58:27.1
139.40401 7.57410 galactic Cam Second-epoch detections are separated by 0.8" and 4.6 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 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 488417294290142080,2461083.9979,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:59.67 +64:58:27.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.92 03:13:44.65 +72:20:21.0
133.34400 12.40886 galactic Cas Second-epoch detections are separated by 5.4" 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 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 12.4979* 03 13 44.65 +72 20 21.0 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 544137588646092544,2461083.9979,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:44.65 +72:20:21.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:27.02 +67:59:46.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.00 03:28:33.98 +67:12:39.8
137.30189 8.83316 galactic Cam Second-epoch detections are separated by 4.3" and 3.9 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 492628423824188032 | 03:28:36.60 +67:12:42.0 (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 492628423824188032,2461083.9979,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 492628423824188032 20260212.4979 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:33.98 +67:12:39.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 488394200250506880,2461083.9979,11.95,0.05,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 488394200250506880 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:51.56 +64:55:14.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.20 03:11:42.74 +72:13:51.7
133.26782 12.23553 galactic Cas Second-epoch detections are separated by 3.3" and 4.4 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 544130059566235136 | 03:11:44.29 +72:13:51.5 (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 12.4979* 03 11 42.74 +72 13 51.7 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 544130059566235136,2461083.9979,12.20,0.05,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 544130059566235136 20260212.4979 12.20CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:42.74 +72:13:51.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 484182112938906496,2461083.9979,11.99,0.05,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
Gaia DR3 484182112938906496 20260212.4979 11.99CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:35.24 +67:04:19.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.97 03:36:10.00 +65:20:47.6
139.02502 7.75963 galactic Cam Second-epoch detections are separated by 2.1" and 4.9 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 488488899984389248 | 03:36:08.67 +65:20:44.0 (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 488488899984389248,2461083.9979,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 488488899984389248 20260212.4979 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:10.00 +65:20:47.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.97 03:35:47.81 +65:19:18.9
139.00829 7.71695 galactic Cam Second-epoch detections are separated by 1.2" and 4.7 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 488487486939478144 | 03:35:46.89 +65:19:16.6 (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 488487486939478144,2461083.9979,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 488487486939478144 20260212.4979 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:47.81 +65:19:18.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.02,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:53.77 +67:02:52.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.23 03:15:44.05 +70:14:31.3
134.62019 10.71762 galactic Cas Second-epoch detections are separated by 2.2" and 4.5 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 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 12.4979* 03 15 44.05 +70 14 31.3 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 541477178525619456,2461083.9979,12.23,0.05,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 541477178525619456 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:44.05 +70:14:31.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.29 04:57:02.30 +71:52:52.4
139.56907 17.51068 galactic Cam Second-epoch detections are separated by 2.7" and 4.1 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 | 04:57:02.30 +71:52:52.4 (user input) | T | P | (position from user input) J-Ks=0.559+/-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,2461083.9979,12.29,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:02.30 +71:52:52.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.18 05:15:53.73 +66:09:33.0
145.51325 15.74856 galactic Cam Second-epoch detections are separated by 1.6" and 4.0 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 481112409613766784 | 05:15:59.14 +66:10:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+66 284 J-Ks=0.350+/-0.036 (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 481112409613766784,2461083.9979,12.18,0.05,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
Gaia DR3 481112409613766784 20260212.4979 12.18CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:53.73 +66:09:33.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.05 03:16:36.21 +71:35:41.8
133.94206 11.89799 galactic Cas Second-epoch detections are separated by 6.7" 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 543863496715339648 | 03:16:38.10 +71:35:38.6 (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 12.4979* 03 16 36.21 +71 35 41.8 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 543863496715339648,2461083.9979,12.05,0.05,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 543863496715339648 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:36.21 +71:35:41.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.07 03:53:46.25 +65:00:41.2
140.70177 8.63697 galactic Cam Second-epoch detections are separated by 1.0" and 4.5 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 489016455107655040 | 03:53:45.60 +65:00:36.4 (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 489016455107655040,2461083.9979,12.07,0.05,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 489016455107655040 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:46.25 +65:00:41.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.04,0.05,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 20260212.4979 12.04CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:31.22 +70:13:21.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.12 03:25:19.25 +68:47:20.5
136.14237 9.96173 galactic Cas Second-epoch detections are separated by 5.2" and 3.5 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 493109941197015424 | 03:25:20.64 +68:47:02.6 (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 12.4979* 03 25 19.25 +68 47 20.5 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 493109941197015424,2461083.9979,12.12,0.05,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 493109941197015424 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:19.25 +68:47:20.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.24 04:29:19.32 +69:15:32.8
140.21755 14.07992 galactic Cam Second-epoch detections are separated by 2.5" and 4.1 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 | 04:29:19.32 +69:15:32.8 (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,2461083.9979,12.24,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:19.32 +69:15:32.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.30 05:17:16.00 +73:34:58.6
138.90534 19.68944 galactic Cam Second-epoch detections are separated by 0.9" and 4.2 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 | 05:17:16.00 +73:34:58.6 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.031 (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,2461083.9979,12.30,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:16.00 +73:34:58.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.15 03:13:50.16 +71:48:22.4
133.63903 11.96063 galactic Cas Second-epoch detections are separated by 7.6" and 5.4 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 543919846686253824 | 03:13:52.42 +71:48:22.4 (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 12.4979* 03 13 50.16 +71 48 22.4 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 543919846686253824,2461083.9979,12.15,0.05,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 543919846686253824 20260212.4979 12.15CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:50.16 +71:48:22.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.09 03:37:57.02 +64:58:27.8
139.40011 7.57147 galactic Cam Second-epoch detections are separated by 2.9" and 4.1 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 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 488417294290142080,2461083.9979,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:57.02 +64:58:27.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:16.68 +72:56:17.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 J035756.26+650223.2,2461083.9979,12.13,0.05,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
ASASSN-V J035756.26+650223.2 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:57.19 +65:02:28.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.48 04:50:22.60 +72:53:50.0
138.39474 17.69227 galactic Cam Second-epoch detections are separated by 0.7" and 4.2 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 | 04:50:22.60 +72:53:50.0 (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,2461083.9979,12.48,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:22.60 +72:53:50.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.34 03:16:54.08 +73:32:39.0
132.88109 13.54996 galactic Cas Second-epoch detections are separated by 6.5" and 5.5 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 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 12.4979* 03 16 54.08 +73 32 39.0 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 544352573231049984,2461083.9979,12.34,0.05,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
Gaia DR3 544352573231049984 20260212.4979 12.34CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:54.08 +73:32:39.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.10 03:49:53.63 +64:58:42.9
140.40376 8.35051 galactic Cam Second-epoch detections are separated by 0.7" and 4.5 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 | ATO J057.4693+64.9773 | 03:49:52.64 +64:58:38.3 (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 J057.4693+64.9773,2461083.9979,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J057.4693+64.9773 20260212.4979 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:53.63 +64:58:42.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.37 05:46:33.73 +65:49:16.6
147.40453 18.31050 galactic Cam Second-epoch detections are separated by 1.6" and 4.1 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 | 05:46:33.73 +65:49:16.6 (user input) | T | P | (position from user input) J-Ks=0.782+/-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,2461083.9979,12.37,0.05,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
target 20260212.4979 12.37CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:33.73 +65:49:16.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.28 03:37:42.79 +64:57:11.5
139.39253 7.53950 galactic Cam Second-epoch detections are separated by 3.5" and 5.1 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 488417534808323840 | 03:37:41.60 +64:57:09.8 (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 488417534808323840,2461083.9979,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 488417534808323840 20260212.4979 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:42.79 +64:57:11.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 12.4979* 03 05 57.14 +73 01 01.3 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
target,2461083.9979,12.46,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:57.14 +73:01:01.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.34 03:37:32.06 +64:51:18.5
139.43604 7.44942 galactic Cam Second-epoch detections are separated by 2.7" and 5.0 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 488392795796736768 | 03:37:30.59 +64:51:13.0 (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 488392795796736768,2461083.9979,12.34,0.05,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
Gaia DR3 488392795796736768 20260212.4979 12.34CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:32.06 +64:51:18.5 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.37 03:39:34.54 +65:09:56.8
139.42283 7.82732 galactic Cam Second-epoch detections are separated by 2.0" and 4.6 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 488426846297294848 | 03:39:33.55 +65:09:54.6 (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 488426846297294848,2461083.9979,12.37,0.05,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 488426846297294848 20260212.4979 12.37CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:34.54 +65:09:56.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.27 03:40:08.33 +65:14:33.3
139.42370 7.92419 galactic Cam Second-epoch detections are separated by 2.1" and 4.9 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 488428907881568640 | 03:40:07.37 +65:14:29.2 (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 488428907881568640,2461083.9979,12.27,0.05,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
Gaia DR3 488428907881568640 20260212.4979 12.27CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:08.33 +65:14:33.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.57,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:21.20 +68:15:00.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.46,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:23.93 +65:27:30.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.39 03:41:00.67 +65:05:58.7
139.58459 7.86568 galactic Cam Second-epoch detections are separated by 1.3" and 4.7 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 488423410323452032 | 03:40:59.47 +65:05:59.2 (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 488423410323452032,2461083.9979,12.39,0.05,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
Gaia DR3 488423410323452032 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:00.67 +65:05:58.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.43 03:38:15.77 +65:04:36.2
139.36518 7.67326 galactic Cam Second-epoch detections are separated by 4.8" and 4.8 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 488420073130142720 | 03:38:14.73 +65:04:34.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 488420073130142720,2461083.9979,12.43,0.05,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
Gaia DR3 488420073130142720 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:15.77 +65:04:36.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 488320292449585920,2461083.9979,12.43,0.05,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
Gaia DR3 488320292449585920 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:13.76 +65:08:27.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.46,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:50.21 +64:55:48.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.56,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:04.42 +64:53:36.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 12.48 03:40:11.42 +64:52:55.7
139.64750 7.63997 galactic Cam Second-epoch detections are separated by 1.8" and 4.6 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 488407536124433280 | 03:40:10.49 +64:52:57.0 (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 488407536124433280,2461083.9979,12.48,0.05,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 488407536124433280 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:11.42 +64:52:55.7 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 J033402.57+652410.4,2461083.9979,12.57,0.05,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
ASASSN-V J033402.57+652410.4 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:04.39 +65:24:17.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.73,0.05,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 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:39.44 +65:22:17.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,12.74,0.05,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
target 20260212.4979 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:33.07 +66:54:49.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,11.24,0.05,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
IK Cam 20260212.4979 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:04.90 +67:38:55.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 J0438053+651356,2461083.9979,9.64,0.05,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
NSVS J0438053+651356 20260212.4979 9.64CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:05.77 +65:14:00.1 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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+661955,2461083.9979,10.85,0.05,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
NSVS J0405390+661955 20260212.4979 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:39.59 +66:19:57.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,11.56,0.05,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 20260212.4979 11.56CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:14.32 +74:55:50.9 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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
GSC 04336-02265,2461083.9979,10.57,0.05,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
GSC 04336-02265 20260212.4979 10.57CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:57.47 +71:18:48.8 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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+691635,2461083.9979,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260212.4979 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:01.60 +69:16:32.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 482110392513737216,2461083.9979,11.95,0.05,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 482110392513737216 20260212.4979 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:21.61 +64:57:31.3 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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,2461083.9979,11.99,0.05,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 20260212.4979 11.99CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:39.23 +69:23:42.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.29 03:28:19.07 +68:29:58.4
136.53711 9.87785 galactic Cas Second-epoch detections are separated by 5.7" and 3.4 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 493042080714160256 | 03:28:20.96 +68:30:01.8 (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 12.4979* 03 28 19.07 +68 29 58.4 11.3 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 493042080714160256,2461083.9979,11.29,0.05,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 493042080714160256 20260212.4979 11.29CV 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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:19.07 +68:29:58.4 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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 J0439483+662343,2461083.9979,11.42,0.05,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
NSVS J0439483+662343 20260212.4979 11.42CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:48.80 +66:23:44.0 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4979 2461083.9979 11.36 03:44:48.31 +65:16:41.2
139.79243 8.25028 galactic Cam Second-epoch detections are separated by 1.8" and 4.7 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 488511130735004672 | 03:44:48.44 +65:16:43.8 (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 488511130735004672,2461083.9979,11.36,0.05,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 488511130735004672 20260212.4979 11.36CV 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:48.31 +65:16:41.2 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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+695613,2461083.9979,11.73,0.05,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
NSVS J0433225+695613 20260212.4979 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/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:22.65 +69:56:11.6 ;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_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20_00sec_-14_90C_LIGHT_0054_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20_00sec_-14_90C_LIGHT_0053_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: 2461083.99819444 12.02.2026 11:57:14.000 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
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: 5 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): 15515
Objects passed selection criteria: 15474
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 12587
Average stars matched: 12212 (97.0207 %)
Memory usage VmPeak: 120428 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 Thu Feb 12 06:00:09 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: 2461083.99819444 12.02.2026 11:57:14.000 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 396
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): 105590
Objects passed selection criteria: 105371
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 84051.2
Average stars matched: 80366.2 (95.6158 %)
Memory usage VmPeak: 1936072 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 Thu Feb 12 06:03:10 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: 1160481 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1160481 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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.png' -> 'transient_report/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits_preview.png'
Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
renamed 'Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.png' -> 'transient_report/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits_preview.png'
Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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= 1703.9427
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 614.1347
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1704.4362
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 613.5990
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.76247
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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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: 2461083.99765101
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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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 04:47:58.563 +69:59:39.64
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 04:47:57.237 +69:59:15.52
Angular distance between the image centers 0.02 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 04:47:58.563 +69:59:39.64
Second-epoch second image center 04:47:57.237 +69:59:15.52
Angular distance between the image centers 0.00696 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.eA0rGU04O8
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.M8SoiakT6T
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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.0Oa3C4iZVn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.M3IXXwGr7Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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 44 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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
2.4 pix Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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
14.3 mag. Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
14.3 mag. Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (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.eA0rGU04O8 (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/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.M8SoiakT6T (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/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.0Oa3C4iZVn (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=685, passed=9170
Got 9170 stars (including 8480 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 9170 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 973 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.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.M3IXXwGr7Y (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=744, passed=9069
Got 9069 stars (including 8320 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 9069 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 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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__out21019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21354.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 7s
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Considering the candidate 21018_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21018_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 21019_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21019_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:21:06.50 +70:35:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 5.037 542980455737217408 050.28129038886 +70.59024579014 10.6516 10.2288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21020_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21020_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:35.72 +66:00:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 4.035 491571346472531968 053.64645963858 +66.00298612523 9.9389 9.4909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21021_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21021_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:29:07.66 +68:07:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.452 492833409723322112 052.28143088211 +68.12533277596 10.1118 9.6448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21023_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21023_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:51:39.08 +65:42:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.827 489857414003291648 057.91074760453 +65.71048326605 10.2351 9.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21024_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21024_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:26:46.84 +68:51:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 3.451 493070839811020032 051.69253722175 +68.86628099855 9.9759 9.5118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21025_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21025_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:23:55.94 +69:57:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 2.959 542756735184021632 050.98089956600 +69.95122794294 9.6884 9.3033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21038_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21038_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:08:48.28 +72:32:54.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21039_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21039_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:12:37.40 +71:33:19.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21064_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21064_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:06:58.91 +72:49:33.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21070_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21070_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:40:28.67 +64:56:56.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21080_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21080_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21082_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21082_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:32.46 +64:48:13.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21102_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21102_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:00:40.38 +65:07:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.13, MAG_FAINT_SEARCH_LIMIT=11.11)GAIADR2_OUTPUT=# 4.781 488988524939522432 060.16595977183 +65.13139105171 9.2124 8.2579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21116_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21116_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:26.14 +64:48:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 2.985 488216324179547008 055.60790993502 +64.80840422083 9.0732 8.6811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21125_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21125_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21134_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21134_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:58:55.94 +64:56:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 3.008 488979728846273024 059.73162839089 +64.93924151799 9.5620 8.6641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21146_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21146_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:55:00.69 +64:53:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 1.352 489012336238076288 058.75228808677 +64.89044125571 9.6965 9.2701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21150_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21150_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21152_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21152_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:57:26.66 +64:57:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.67, MAG_FAINT_SEARCH_LIMIT=11.65)GAIADR2_OUTPUT=# 3.062 489004738436872576 059.35964562691 +64.95943331686 9.7301 8.8338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:51:52.24 +65:02:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 0.168 488269822292126592 057.96775222739 +65.04772054889 9.7857 9.4008 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 21155_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21155_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:12:48.04 +73:28:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 1.965 544359896152218240 048.20176946108 +73.47135576284 9.6647 9.1605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21164_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21164_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:57:15.33 +64:56:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 0.806 489004605296884480 059.31391361461 +64.93386002766 9.9363 9.4868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21175_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21175_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:19.49 +64:51:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 3.388 488439555100930816 053.83202650346 +64.85834668395 9.4340 9.1339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21191_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21191_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:56:39.18 +64:52:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 3.559 489002921669734272 059.16154151417 +64.87016196399 9.9784 9.0401 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#
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Considering the candidate 21194_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21194_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:12.78 +64:57:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 2.540 488406745850400256 055.30268973101 +64.95810886615 9.4348 9.0861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21211_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21211_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21224_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21224_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21230_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21230_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21261_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21261_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:05.18 +64:51:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 4.513 488252058307506176 057.01882878442 +64.86285592315 10.0092 8.7279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:51.18 +65:01:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.738 488407433045118720 055.46080378841 +65.03133676110 10.1313 9.2605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21280_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21280_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:33.16 +64:44:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 2.503 488387916713924736 054.38653942256 +64.73336572178 9.9402 9.0135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21300_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21300_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:18.83 +64:48:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 2.894 488248755473094912 057.07714987016 +64.80914249617 10.3820 9.3020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21315_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21315_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 21320_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21320_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:39.64 +65:20:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.495 491467305185081984 053.66469780486 +65.33986621149 10.2874 9.7717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21321_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21321_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:36:58.64 +64:57:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.901 488464710728708096 054.24575591289 +64.96201191914 10.2498 9.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21343_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21343_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:45:43.76 +64:55:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 3.210 488302360964201344 056.43025187650 +64.92485130864 10.4317 9.4664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21352_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21352_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:44:01.01 +69:06:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.984 496311856496236800 071.00549774881 +69.10413684241 12.0561 11.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21354_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 21354_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21376_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21376_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:01.22 +65:11:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 3.119 489772751608416384 058.25389184967 +65.19807021850 10.7226 9.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21405_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 21405_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:53:47.21 +70:14:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.318 497226061756783360 073.44696960334 +70.24650470381 12.2945 11.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07347_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 07347_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10157_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 10157_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12327_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 12327_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 26s
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 ####
03:56:58.17 +70:34:27.9
03:43:03.98 +68:35:28.1
03:39:14.87 +65:13:13.0
03:54:14.31 +65:06:44.3
03:35:50.78 +65:16:35.6
03:15:00.22 +70:30:11.4
03:36:12.01 +65:29:18.6
03:13:42.44 +71:37:45.0
03:44:54.11 +65:03:16.0
03:56:25.35 +65:16:19.9
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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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 04:47:58.563 +69:59:39.64
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 04:47:57.237 +69:59:15.52
Angular distance between the image centers 0.02 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 04:47:58.563 +69:59:39.64
Second-epoch second image center 04:47:57.237 +69:59:15.52
Angular distance between the image centers 0.00696 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.tKT8rUgRrg
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.ChJnqJc9ee
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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.HC9Rts7N3C
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.2elUNOUch1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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 351 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
2.5 pix Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
2.4 pix Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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
13.2 mag. Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
13.2 mag. Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.6 (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.tKT8rUgRrg (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/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.ChJnqJc9ee (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/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.HC9Rts7N3C (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3795, passed=55746
Got 55746 stars (including 51884 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 55746 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 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.48"
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_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-56-27_20.00sec_-14.90C_LIGHT_0053.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.2elUNOUch1 (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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3987, passed=56491
Got 56491 stars (including 52427 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 56491 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 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: 0.48"
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 975 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: 0.47"
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_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q2b1x1_055800_TTUQ2b1x1_765_MoM2AXeB/Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054.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__out132928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out133738.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out134054.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out02028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92128.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 209s
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: 77s
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Considering the candidate 132928_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132928_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:27:55.24 +73:53:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.280 544709987527189760 051.97992700454 +73.88662383782 13.0744 12.5234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132929_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132929_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:47:17.97 +69:03:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.809 494446053983013760 056.82765920910 +69.06511383209 13.3670 12.6673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132934_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132934_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:20.03 +71:19:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.679 542956747517402880 053.83437106633 +71.32546081778 13.1857 12.2770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132937_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132937_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:23:33.49 +70:55:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.340 543021137667331840 050.88964096844 +70.92175548512 12.8619 12.1885 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 132938_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132938_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:26:34.03 +71:04:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.439 543111572498670976 051.64050644179 +71.08058194957 12.6559 12.0147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132940_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132940_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:26:59.41 +69:03:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.232 493121451709220992 051.74512517372 +69.05982887019 12.4355 11.7391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132941_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132941_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132944_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132944_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:36:08.98 +66:23:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.678 491674631846172800 054.03715736611 +66.38379603357 12.4319 11.6779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132945_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132945_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132946_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132946_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:18:04.88 +71:09:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 5.668 543069172581349888 049.52487860514 +71.16440186410 12.4766 11.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132947_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132947_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 06:00:30.71 +65:42:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.850 1008759213627081600 090.12919375797 +65.70278610271 13.4964 12.7385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132948_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132948_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132951_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132951_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:47:12.15 +66:23:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.877 490138236145579520 056.80243176487 +66.38997793529 12.4043 11.8283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132952_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132952_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:14:36.34 +71:48:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.627 543917304065614848 048.65050245852 +71.80331146864 12.1514 11.4969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132955_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132955_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:23:17.46 +69:14:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.526 541173919475536000 050.82300629627 +69.23730871586 12.2318 11.6544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132958_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132958_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132959_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132959_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:19:05.28 +71:41:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.935 543859888942806912 049.77058517959 +71.68770542586 12.1946 11.5770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132960_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132960_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:23:51.15 +68:53:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.636 493114987779200384 050.96590541690 +68.89710589297 12.0431 11.4200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132961_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132961_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132964_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132964_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:14:41.95 +65:51:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.311 489302950904330112 063.67478238393 +65.86299715579 12.8948 12.0360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132965_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132965_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132966_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132966_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132967_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132967_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132968_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132968_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132969_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132969_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:26:23.52 +73:34:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 5.133 544670302029463296 051.59300346259 +73.57419724201 12.4490 11.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132970_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132970_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:24:16.49 +70:29:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.809 542811642044447616 051.07187397455 +70.49526988346 12.0672 11.6158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132971_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132971_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:28:48.97 +68:20:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.815 492851963982029696 052.20456541030 +68.34728432376 11.7603 11.1364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132973_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132973_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:44:37.60 +65:25:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.751 488516147256742912 056.15538890115 +65.42960488860 11.8120 11.3017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132975_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132975_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132976_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132976_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132977_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132977_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132979_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132979_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:29:14.29 +68:27:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 0.417 492853754987340160 052.30925765263 +68.45997729114 11.8121 11.3726 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 132981_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132981_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:31:05.26 +67:31:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 5.602 492732632610715904 052.77565761184 +67.53272528931 11.9596 11.1099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132983_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132983_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132984_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132984_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132986_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132986_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:23:19.36 +73:07:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 5.355 544278768514463232 050.82562554607 +73.12404454442 11.7790 11.1985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132987_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132987_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132988_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132988_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:51:25.69 +65:58:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 4.759 490057486460719872 057.85678027644 +65.97678992418 12.1825 11.3693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132990_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132990_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:45.02 +66:47:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 5.734 491891093899132672 053.69112499140 +66.78810030076 11.3923 10.9939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132991_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132991_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132992_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132992_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 132993_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132993_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132995_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 132995_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 132996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:22:01.39 +73:08:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 1.904 544279563084247552 050.50621990019 +73.14365303457 11.0500 10.6040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132998_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 132998_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:29:49.18 +68:35:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 1.779 493048368546265344 052.45381395781 +68.59959258534 10.6026 10.2336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133001_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133001_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:29:07.93 +68:07:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 2.270 492833409723322112 052.28143088211 +68.12533277596 10.1118 9.6448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133002_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133002_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:51:39.21 +65:42:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.96, MAG_FAINT_SEARCH_LIMIT=10.94)GAIADR2_OUTPUT=# 4.770 489857414003291648 057.91074760453 +65.71048326605 10.2351 9.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133003_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133003_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 133005_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133005_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:20:06.04 +69:43:51.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133014_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133014_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:16:38.77 +69:58:43.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133021_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133021_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:08:48.10 +72:32:54.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133054_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133054_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:06:58.63 +72:49:33.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133055_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133055_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:40:28.78 +64:56:55.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133059_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133059_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:14.87 +65:13:13.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133067_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133067_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:15:10.51 +70:33:04.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133068_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133068_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:30:48.68 +64:51:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.74, MAG_FAINT_SEARCH_LIMIT=9.72)GAIADR2_OUTPUT=# 0.796 477013468924148736 067.70271900409 +64.86395099587 9.4941 8.8644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133075_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133075_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:32.47 +64:48:13.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 133094_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133094_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:00:40.36 +65:07:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.00, MAG_FAINT_SEARCH_LIMIT=9.98)GAIADR2_OUTPUT=# 4.109 488988524939522432 060.16595977183 +65.13139105171 9.2124 8.2579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133113_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133113_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:54:14.40 +65:06:44.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133120_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133120_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133126_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133126_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:58:56.01 +64:56:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.34, MAG_FAINT_SEARCH_LIMIT=10.32)GAIADR2_OUTPUT=# 3.289 488979728846273024 059.73162839089 +64.93924151799 9.5620 8.6641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133148_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133148_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:55:00.60 +64:53:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.49, MAG_FAINT_SEARCH_LIMIT=10.47)GAIADR2_OUTPUT=# 0.342 489012336238076288 058.75228808677 +64.89044125571 9.6965 9.2701 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 133152_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133152_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:57:26.71 +64:57:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.55, MAG_FAINT_SEARCH_LIMIT=10.53)GAIADR2_OUTPUT=# 3.233 489004738436872576 059.35964562691 +64.95943331686 9.7301 8.8338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133156_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133156_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:50.81 +65:16:35.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133158_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133158_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133162_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133162_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:51:52.31 +65:02:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.61, MAG_FAINT_SEARCH_LIMIT=10.59)GAIADR2_OUTPUT=# 0.429 488269822292126592 057.96775222739 +65.04772054889 9.7857 9.4008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133164_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133164_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:12.48 +64:57:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.76, MAG_FAINT_SEARCH_LIMIT=10.74)GAIADR2_OUTPUT=# 5.004 488406745850400256 055.30268973101 +64.95810886615 9.4348 9.0861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133168_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133168_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:21:50.35 +70:12:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.70, MAG_FAINT_SEARCH_LIMIT=10.68)GAIADR2_OUTPUT=# 4.373 542778454835268224 050.46337088664 +70.20260486409 9.8102 9.4729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133178_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133178_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:57:15.39 +64:56:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.65, MAG_FAINT_SEARCH_LIMIT=10.63)GAIADR2_OUTPUT=# 0.774 489004605296884480 059.31391361461 +64.93386002766 9.9363 9.4868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133197_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133197_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133203_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133203_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133208_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133208_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:56:39.24 +64:52:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)GAIADR2_OUTPUT=# 3.848 489002921669734272 059.16154151417 +64.87016196399 9.9784 9.0401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133214_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133214_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:15:00.15 +70:30:10.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133218_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133218_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:19.53 +64:51:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.87, MAG_FAINT_SEARCH_LIMIT=10.85)GAIADR2_OUTPUT=# 4.461 488439555100930816 053.83202650346 +64.85834668395 9.4340 9.1339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133242_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133242_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133255_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133255_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:12:50.30 +72:38:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.15, MAG_FAINT_SEARCH_LIMIT=11.13)GAIADR2_OUTPUT=# 3.887 544250563465033728 048.21279981121 +72.63791108410 10.0998 9.6185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133258_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133258_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:12:52.79 +64:56:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.04, MAG_FAINT_SEARCH_LIMIT=11.02)GAIADR2_OUTPUT=# 5.426 488828923953788544 063.21739765602 +64.94700869038 10.0740 8.6680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:36:12.07 +65:29:18.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133290_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133290_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133297_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133297_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:05.26 +64:51:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.13, MAG_FAINT_SEARCH_LIMIT=11.11)GAIADR2_OUTPUT=# 5.025 488252058307506176 057.01882878442 +64.86285592315 10.0092 8.7279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133299_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133299_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:13:41.43 +71:37:47.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133316_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133316_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133326_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133326_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133333_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133333_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:51.28 +65:01:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 4.352 488407433045118720 055.46080378841 +65.03133676110 10.1313 9.2605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133358_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133358_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:18.92 +64:48:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 3.318 488248755473094912 057.07714987016 +64.80914249617 10.3820 9.3020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133359_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133359_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:33.17 +64:43:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 3.086 488387916713924736 054.38653942256 +64.73336572178 9.9402 9.0135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133375_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133375_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:58:05.89 +65:03:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.32, MAG_FAINT_SEARCH_LIMIT=11.30)GAIADR2_OUTPUT=# 1.761 489029172509762176 059.52353268704 +65.06625867069 10.6777 10.0190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133416_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133416_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:56:25.48 +65:16:19.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133417_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133417_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:44:54.16 +65:03:15.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 133430_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133430_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133434_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133434_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133438_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133438_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133439_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133439_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133441_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133441_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:45:43.83 +64:55:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 3.869 488302360964201344 056.43025187650 +64.92485130864 10.4317 9.4664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133443_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133443_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133451_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133451_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133461_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133461_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:27:10.82 +72:14:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 2.686 543989566892653440 051.79720287348 +72.24440036801 10.8317 10.2858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133466_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133466_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:36:58.47 +64:57:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.58, MAG_FAINT_SEARCH_LIMIT=11.56)GAIADR2_OUTPUT=# 5.748 488464710728708096 054.24575591289 +64.96201191914 10.2498 9.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133467_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133467_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:22:24.80 +71:53:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.968 543954588679079808 050.60367202426 +71.88525869061 10.8648 10.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133468_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133468_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:39.71 +65:20:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 2.063 491467305185081984 053.66469780486 +65.33986621149 10.2874 9.7717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133477_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133477_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:01.31 +65:11:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 3.332 489772751608416384 058.25389184967 +65.19807021850 10.7226 9.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133488_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133488_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133494_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133494_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:51.40 +64:53:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 4.673 488440040436618496 053.96211643078 +64.88474084617 10.2531 9.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133504_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133504_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:06:30.81 +73:13:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 4.542 547238692472995712 046.63274677533 +73.22742699748 10.7271 10.2531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133541_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133541_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:40:28.57 +65:14:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.866 488428220682947712 055.11853392747 +65.23891782346 10.6310 10.1463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133546_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133546_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133556_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133556_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133560_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133560_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:04.87 +65:20:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 4.309 488480069531584640 054.76769793068 +65.34382139274 10.6476 9.7443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133563_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133563_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:23.64 +65:01:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 5.767 488410284903420288 055.34483099249 +65.01639930897 10.7395 9.7392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133570_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133570_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:04:18.00 +73:20:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)
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Considering the candidate 133573_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133573_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:28.82 +65:08:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 4.338 488505667536738944 055.36783408725 +65.13796889722 10.7051 10.2460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133583_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133583_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133588_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133588_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133591_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133591_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133596_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133596_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:38.03 +65:12:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 4.491 488473919138463872 054.65568636781 +65.20588040991 10.6797 9.8446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133599_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133599_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:55:57.07 +65:03:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 0.644 489019723581753856 058.98739694880 +65.05293425887 11.1837 10.6691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133607_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133607_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133609_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133609_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133613_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133613_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133614_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133614_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:58:46.23 +65:02:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 2.738 489028554034464896 059.69193849551 +65.04479668395 11.2784 10.6760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133633_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133633_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133636_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133636_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:08:52.43 +72:50:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 3.145 544213450650464000 047.22137794136 +72.83813230323 11.1879 10.7981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133639_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133639_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:49.34 +65:09:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 1.800 488426056023307520 054.95540970197 +65.16116118763 10.7955 10.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133647_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133647_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:46:05.40 +65:27:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 3.683 488536866178926080 056.52081158907 +65.46250495472 11.0484 10.0380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133667_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133667_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:44:20.28 +65:03:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 3.155 488313699677845504 056.08507788105 +65.05650850832 11.0470 10.5847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133675_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133675_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 05:03:07.88 +66:49:09.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133678_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133678_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:40.76 +64:49:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 3.331 488438700406853376 053.91780929997 +64.82895033806 10.6047 9.8088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133694_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133694_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:12.65 +64:45:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 3.120 488400114421025792 054.55120970757 +64.75814080652 10.6640 9.7578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133706_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133706_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:59.94 +65:15:41.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)
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Considering the candidate 133731_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133731_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:02.36 +64:42:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 5.446 488376234402879744 054.50981924856 +64.70584621252 10.8105 10.2432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133738_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133738_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:50:34.47 +64:52:48.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)
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Considering the candidate 133767_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133767_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:45.78 +65:28:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 5.240 488493469829519232 054.68744068606 +65.47754632470 11.0655 10.1249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133783_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133783_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133804_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133804_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:16:15.59 +70:05:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 5.301 541460445333041152 049.06877229222 +70.09222261740 11.0560 10.6046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133821_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133821_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:08:42.64 +72:28:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 5.151 544151882294427392 047.18241499336 +72.46837728395 11.3575 10.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133823_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133823_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133831_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133831_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:13:36.51 +73:37:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 2.559 544363229046824448 048.40456131012 +73.61684815622 11.4527 10.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133842_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133842_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:04.10 +64:53:01.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)
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Considering the candidate 133861_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133861_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:00:17.62 +64:58:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 2.039 488978698052713856 060.07218023205 +64.97089417249 11.5522 10.6480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133864_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133864_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133883_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133883_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133889_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133889_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:13:40.98 +72:09:22.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133892_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133892_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:47:20.24 +64:50:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 3.613 488252608063036672 056.83513992355 +64.84902666092 11.3145 10.8308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133896_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133896_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:22.78 +65:28:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 3.426 491495205292581888 053.59262665610 +65.47198919428 10.9380 10.3989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133897_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133897_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:56.90 +65:22:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.639 488526592617272192 055.73599622556 +65.38128787782 11.3971 10.6006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133902_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133902_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:02:55.22 +65:03:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 3.556 488973406654622848 060.72836110749 +65.04941407263 11.6932 10.5939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133905_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133905_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133922_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133922_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133944_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133944_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133955_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133955_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133961_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133961_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133963_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133963_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 133964_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133964_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133995_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133995_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:43:45.16 +64:54:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 5.756 488308167760031232 055.93442569080 +64.90033258907 11.1127 9.7361 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 133997_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 133997_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:39.26 +64:52:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 5.308 488217148813256960 055.66011601107 +64.86770308496 11.3484 10.1101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133999_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 133999_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134026_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134026_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134042_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134042_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:46:46.03 +64:47:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 3.607 488250993155363200 056.69259389003 +64.80016425339 11.4686 10.9617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134053_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134053_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134054_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134054_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:43:14.22 +64:51:51.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)
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Considering the candidate 134060_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134060_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:22:55.95 +69:58:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.963 542759209085183360 050.73524255211 +69.97036146892 11.5559 11.0549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134069_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134069_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:53.61 +64:59:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 5.742 488407123807489152 055.46966188828 +64.98968928861 11.2986 10.3209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134070_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134070_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134073_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134073_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:22:55.05 +72:08:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 2.758 543979052812758912 050.73130708103 +72.13479102220 11.6765 11.0719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134085_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134085_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:46.56 +65:26:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 5.280 491492044196658816 053.69064490068 +65.43871270931 11.3722 10.4402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134100_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134100_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134103_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134103_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:24:01.23 +73:56:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 4.077 544760801283177856 051.00885698205 +73.93804817753 11.8224 11.3133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134107_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134107_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:24.85 +65:10:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 2.059 488517521643401856 055.35320228900 +65.17335948873 11.4464 10.8216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134114_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134114_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:09.30 +65:18:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 2.601 488488006631917824 053.78793566105 +65.31008175739 11.1699 10.5767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134120_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134120_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134146_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134146_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134148_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134148_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134158_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134158_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:16.33 +65:18:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.050 488522469448745088 055.31873299205 +65.31020982614 11.8942 11.1099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134187_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134187_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134191_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134191_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134198_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134198_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:03:11.03 +65:02:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 3.413 489064219442981248 060.79427174469 +65.04431794276 12.0623 11.0149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134200_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134200_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134207_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134207_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:45:34.96 +64:46:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 2.994 488291846884311296 056.39405552362 +64.77374714886 11.5664 10.6159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134215_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134215_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134229_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134229_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:13:32.46 +72:06:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134240_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134240_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134242_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134242_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134243_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134243_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:52:34.54 +64:55:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 4.326 488265183727468800 058.14143580735 +64.92872342289 11.9789 11.2473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134253_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134253_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:21.95 +64:59:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.760 489016012729799168 058.34084131628 +64.99355864420 12.0250 11.2671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134262_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134265_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134265_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:58.78 +65:15:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 4.706 488464229692294016 053.74192016635 +65.26471329562 11.3803 10.5115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134267_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134267_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134271_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134271_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:00.28 +64:47:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 4.715 488399702100658816 054.75040723094 +64.78901910113 11.3768 10.6576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134274_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134274_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:24.07 +65:19:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 3.327 488338541768547584 057.09810789003 +65.31982184728 11.6416 10.6569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134275_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134275_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:50:35.30 +65:05:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 4.375 488281985639517312 057.64490358991 +65.09792554640 11.7365 10.5863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134280_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134280_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:19:43.56 +73:30:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.986 544349210273680640 049.93346420421 +73.51337341368 11.9725 11.4620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134283_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134283_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:56:37.55 +65:04:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 2.615 489021201050486016 059.15503040846 +65.07706520776 12.0222 11.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134285_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134285_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:59:41.00 +64:55:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.033 488978182658338944 059.92015671451 +64.92562865571 12.1749 11.4801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134290_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134290_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:43:25.95 +65:12:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.483 488504155708186496 055.85808837432 +65.20496719229 11.6637 10.7704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134299_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134299_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134302_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134302_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134317_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134317_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:43.16 +64:44:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 4.430 488212201011316480 055.67736897839 +64.73766679550 11.6343 10.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134328_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134328_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134346_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134346_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134353_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134353_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:22:03.71 +70:36:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.956 542981138634153984 050.51950750165 +70.61607613009 11.9583 11.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134357_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134357_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:46.89 +65:14:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 4.324 488518449359372672 055.44255231879 +65.24303707461 11.6453 10.6887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134358_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134358_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:25.09 +65:02:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 4.811 488465569722121984 054.35141799688 +65.04772286211 11.5679 10.5919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134361_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134361_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:56.98 +64:58:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 4.484 488442033301408256 053.98964510377 +64.96778620914 11.1424 10.6444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134362_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134362_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134363_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134363_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134365_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134365_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134393_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134393_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134410_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134410_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:56.50 +65:09:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 3.408 488506560889902976 055.73495213734 +65.16750977883 11.8161 11.1001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134411_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134411_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:36.23 +65:11:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 4.398 488426945077807360 054.89806471142 +65.19677708995 11.6551 11.0408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134414_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134414_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:11:16.96 +72:34:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.499 544157826531945472 047.82236602165 +72.57288861575 12.3517 11.9619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134434_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134434_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134436_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134436_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:34.70 +64:50:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 1.141 489011374165131648 058.39519762886 +64.84912588101 12.0684 11.4023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134454_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134454_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134462_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134462_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:33.11 +65:07:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.498 488467562587298816 054.63773917404 +65.13279465625 11.7523 11.2176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134465_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134465_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:44.81 +64:53:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 5.563 488416469656453376 054.43307958895 +64.89777168313 11.5626 10.7960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134468_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134468_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134470_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134470_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134480_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134480_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134483_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134483_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134497_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134497_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:36:50.48 +64:53:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 5.362 488393998387176448 054.20682396370 +64.89673583591 11.4929 10.5609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134536_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134536_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134540_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134540_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134543_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134543_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134545_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134545_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:44:08.39 +65:02:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 2.806 488313768397095424 056.03311199346 +65.03943439364 11.8185 10.8887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134558_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134558_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134561_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134561_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:43.00 +64:52:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.131 489011576024810880 058.42922709250 +64.88204802495 12.2575 11.6897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134562_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134562_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:13:45.64 +73:35:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 5.685 544362954168918144 048.44551453445 +73.59870456051 12.0159 11.4634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134564_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134564_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134571_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134571_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134574_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134574_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134587_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134587_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134589_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134589_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134594_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134594_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 05:37:29.08 +66:41:33.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134596_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134596_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134598_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134598_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:40.25 +65:13:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 3.690 488331188784558464 057.16530045542 +65.21809853538 12.1705 11.1113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134599_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134599_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:16:25.69 +72:59:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 5.405 544262207119129984 049.11216280157 +72.98375567250 11.9226 11.3054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134600_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134600_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134657_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134657_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134667_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134667_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:16:47.56 +72:53:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.461 544260626571167488 049.20020613502 +72.88855640306 12.3377 11.7500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134678_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134678_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134682_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134682_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:40.71 +65:08:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 3.906 488506423450959488 055.66706826591 +65.14646122443 12.1277 11.1791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134684_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134684_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:20:38.36 +65:07:05.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134696_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134696_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134701_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134701_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:19:21.64 +73:42:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 5.486 544730534650618240 049.84499494153 +73.71481028389 11.9535 11.4441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134707_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134707_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134719_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134719_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134720_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134720_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134722_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134722_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134731_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134731_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:43:24.40 +64:57:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.145 488311466294636672 055.85037264836 +64.95340083658 11.8311 11.1168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134736_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134736_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:08:34.19 +65:01:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.173 488888224563881728 062.14121940147 +65.02716006416 12.2031 10.8133 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 134738_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134738_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134757_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134757_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134767_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134767_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:09:34.17 +72:28:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.184 544151396962993024 047.39220010441 +72.47279674097 12.3198 11.7543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134769_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134769_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:10:27.77 +66:37:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.379 489586998563101824 062.61513626809 +66.62532740548 12.1607 10.5140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134775_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134775_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:29.06 +65:12:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.661 489773468863335296 058.37126824653 +65.20223970665 12.3986 11.6312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134777_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134777_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134786_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134786_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:57.18 +65:25:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.729 488571668295733888 054.98582586396 +65.42054059749 12.5663 11.3850 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 134837_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134837_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134843_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134843_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:45.08 +64:56:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.066 488403034998694400 054.93704633400 +64.93980148478 11.9313 11.2854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134868_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134868_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:10:16.53 +72:34:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.260 544158445006848896 047.57094823819 +72.58198424581 12.4099 11.8533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134877_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134877_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134893_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134893_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:52.94 +64:55:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.853 488417083832031616 054.46955947474 +64.92827413298 11.7917 11.1327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134895_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134895_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134913_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134913_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134924_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 134924_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 134969_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134969_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134971_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134971_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:40:10.16 +65:16:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.463 488429010960779136 055.03967744035 +65.26772801343 12.1212 11.2649 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 134977_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134977_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 134996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 134996_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:42:59.89 +64:46:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 4.145 488212712109369344 055.74733530950 +64.77344229410 12.0138 10.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135003_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135003_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:44.45 +64:46:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 4.052 488397984117217280 054.93430982899 +64.76839183846 11.6753 11.1002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135005_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135005_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:15:05.96 +70:35:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.682 541538441940524160 048.77694708219 +70.58910948363 12.3033 11.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135013_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135013_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135026_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135026_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135033_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135033_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:54:48.15 +64:55:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.806 489012679835451008 058.69938305659 +64.92803618586 12.4101 11.6396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135072_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135072_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:30.08 +64:59:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.755 488418252064016768 054.37253600728 +64.99313381165 12.0939 11.1191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135077_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135077_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135080_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135080_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135098_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135098_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:48:57.42 +65:03:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.044 488279271220224256 057.23905467612 +65.05727804473 12.4605 11.7349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135099_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135099_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:47:22.28 +64:47:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.169 488251439831950592 056.84011430091 +64.79999532522 12.4697 11.3235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135123_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135123_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:52:17.41 +64:50:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 4.711 487513839329749504 058.06984199270 +64.84423232991 12.5352 11.5586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135155_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135155_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:09:56.42 +72:42:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.377 544207304554776704 047.48718068132 +72.71250395503 12.4790 11.9675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135175_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135175_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 135204_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135204_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135208_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135208_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:07:02.80 +72:36:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.497 544202902210796160 046.76574693555 +72.61450603192 12.2789 11.8266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135218_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135218_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:37:25.09 +64:44:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 4.873 488388191591829120 054.35433771298 +64.74818414068 11.8970 11.2816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135246_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135246_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:18:04.19 +72:49:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.364 544244997187485568 049.52133079571 +72.82773603889 12.3414 11.6382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135255_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135255_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:46:39.12 +65:10:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 2.000 488341805943756928 056.66167624873 +65.18113711318 12.4610 11.3459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135260_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135260_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:46:45.20 +65:06:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.417 488306209254825216 056.68795110148 +65.11101882016 12.2803 11.6962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135263_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135263_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135267_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135267_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 04:02:50.50 +64:57:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.575 488969936321070464 060.70744593063 +64.96490111130 12.8807 11.6933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135305_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135305_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135324_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135324_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:39:54.10 +65:14:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 4.062 488428804802354432 054.97281173801 +65.24790576597 12.3233 11.4916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135346_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135346_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:38:13.91 +64:47:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.767 488411899811277568 054.55817948517 +64.78426277398 12.0144 11.3565 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 135349_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135349_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 135378_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135378_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135409_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135409_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:49:20.43 +64:48:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 4.470 488259991107541120 057.33373503186 +64.81410267356 12.5223 11.4681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135415_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135415_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:34:54.97 +65:03:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.360 488456807988895616 053.72915075725 +65.05029162971 12.0029 11.3912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135430_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135430_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 135455_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135455_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135467_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135467_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135484_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135484_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135512_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135512_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135530_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135530_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135531_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135531_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:09:33.67 +73:12:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.108 544327662420717568 047.38944160496 +73.20789262849 12.4509 11.6469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135541_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135541_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:50:50.93 +64:57:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 5.480 488268069945510656 057.70955268657 +64.96064012991 12.4529 11.3756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135552_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135552_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 135562_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135562_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135575_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135575_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135586_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135586_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135600_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135600_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:47:11.85 +64:55:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.672 488300333739908992 056.79702543895 +64.92666525921 12.7700 11.6894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135634_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135634_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:53:38.88 +64:55:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.547 489014844498697856 058.40919162406 +64.93268726863 12.6494 11.7874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135684_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135684_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:35:04.45 +65:27:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.699 491492250355074176 053.76808838296 +65.45004677674 12.1378 11.4674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135686_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135686_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 135702_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135702_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 06:20:44.56 +72:07:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.845 1113727630225334912 095.18689061982 +72.11776271323 13.6861 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135778_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135778_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:41:56.08 +64:46:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.556 488214743631593216 055.48341417814 +64.77370398469 12.3783 11.6889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135805_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135805_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:45:20.90 +65:08:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.501 488321705496844288 056.33345169286 +65.13852144788 12.4860 11.5851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135836_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135836_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:50:15.36 +65:10:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.253 488286108808106880 057.56678276377 +65.17513072788 13.1468 12.4814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135853_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135853_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 135861_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135861_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:08:59.53 +72:54:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.983 544225442198980096 047.24651471496 +72.90101400490 12.4767 11.8072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135862_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 135862_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135873_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135873_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 135918_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135918_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 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 135994_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 135994_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136041_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 136041_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136121_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 136121_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136235_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 136235_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136365_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 136365_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 136442_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 136442_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77457_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 77457_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50504_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 50504_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 36122_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 36122_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72831_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 72831_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59521_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 59521_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 90043_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02028_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 02028_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 87153_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89626_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 89626_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 42617_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 42617_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62200_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 62200_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71635_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 71635_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79557_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 79557_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:43:04.14 +68:35:27.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61312_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 61312_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80997_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 80997_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50982_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 50982_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 03:56:58.23 +70:34:27.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76885_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 76885_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92128_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 92128_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06691_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
The candidate 06691_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73802_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 73802_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58701_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 58701_Cam-06-Q2b1x1_2026-02-12_05-57-14_20.00sec_-14.90C_LIGHT_0054
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 305s
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 ####
03:56:58.17 +70:34:27.9
03:43:03.98 +68:35:28.1
03:39:14.87 +65:13:13.0
03:54:14.31 +65:06:44.3
03:35:50.78 +65:16:35.6
03:15:00.22 +70:30:11.4
03:36:12.01 +65:29:18.6
03:13:42.44 +71:37:45.0
03:44:54.11 +65:03:16.0
03:56:25.35 +65:16:19.9
05:03:14.32 +74:55:50.9
04:32:14.46 +65:36:03.8
03:35:25.28 +67:46:27.5
03:19:57.13 +73:32:31.8
04:22:39.89 +68:29:26.3
03:41:15.95 +66:16:44.3
04:15:51.63 +65:54:40.4
03:28:48.37 +69:27:28.7
03:22:29.99 +70:00:50.4
03:23:14.61 +70:01:35.0
05:44:01.24 +68:13:19.6
03:32:19.85 +67:40:17.6
03:43:00.94 +66:17:03.1
05:10:02.21 +68:35:20.7
03:42:25.66 +64:48:24.0
03:19:32.15 +69:24:55.3
03:12:46.84 +73:28:15.2
03:43:46.25 +65:17:29.2
03:13:37.14 +70:50:51.2
03:24:41.48 +68:45:11.8
03:23:08.24 +69:38:53.2
03:13:11.66 +72:36:29.3
03:17:43.97 +72:32:06.5
03:22:54.84 +68:33:48.0
03:19:43.93 +69:27:22.1
03:21:05.38 +70:35:23.4
03:18:31.95 +71:59:23.6
03:27:41.45 +67:32:24.1
03:38:54.28 +65:23:50.6
03:11:44.36 +71:39:22.9
03:11:35.67 +71:41:32.4
05:02:20.34 +72:25:34.8
03:11:12.76 +71:36:40.6
03:36:18.86 +64:54:29.2
03:36:16.45 +64:54:22.5
04:51:34.01 +68:12:02.3
04:42:14.55 +69:04:10.5
03:11:06.49 +72:08:33.3
04:51:32.82 +68:11:46.1
03:17:24.50 +71:45:17.0
05:13:54.01 +67:29:16.7
04:18:40.76 +74:39:10.7
03:14:16.07 +70:32:08.8
03:30:00.25 +67:45:04.3
03:35:27.04 +65:32:13.9
03:19:36.54 +72:06:51.2
03:16:06.92 +72:04:22.5
04:57:37.86 +70:38:34.7
03:38:42.01 +65:20:21.7
03:16:27.35 +72:23:52.9
03:07:46.27 +72:53:43.2
04:02:57.94 +72:49:32.9
03:35:20.92 +65:32:13.2
05:20:28.75 +71:45:06.8
03:25:28.24 +67:58:18.1
03:41:10.31 +65:18:53.6
03:39:47.90 +64:48:07.8
03:35:48.57 +64:54:50.6
03:08:43.30 +72:37:12.3
05:58:41.51 +66:36:24.1
03:22:50.05 +73:24:19.5
04:47:21.97 +70:17:06.1
05:14:25.32 +69:50:42.1
03:11:51.22 +73:33:27.1
03:10:17.27 +72:32:36.5
03:15:50.18 +73:22:59.9
03:35:46.07 +64:54:43.9
03:27:15.02 +67:49:32.8
03:34:48.29 +65:06:05.0
03:37:59.67 +64:58:27.1
03:13:44.65 +72:20:21.0
05:19:27.02 +67:59:46.9
03:28:33.98 +67:12:39.8
03:36:51.56 +64:55:14.4
03:11:42.74 +72:13:51.7
05:22:35.24 +67:04:19.9
03:36:10.00 +65:20:47.6
03:35:47.81 +65:19:18.9
05:21:53.77 +67:02:52.9
03:15:44.05 +70:14:31.3
04:57:02.30 +71:52:52.4
05:15:53.73 +66:09:33.0
03:16:36.21 +71:35:41.8
03:53:46.25 +65:00:41.2
05:26:31.22 +70:13:21.3
03:25:19.25 +68:47:20.5
04:29:19.32 +69:15:32.8
05:17:16.00 +73:34:58.6
03:13:50.16 +71:48:22.4
03:37:57.02 +64:58:27.8
04:50:16.68 +72:56:17.1
03:57:57.19 +65:02:28.5
04:50:22.60 +72:53:50.0
03:16:54.08 +73:32:39.0
03:49:53.63 +64:58:42.9
05:46:33.73 +65:49:16.6
03:37:42.79 +64:57:11.5
03:05:57.14 +73:01:01.3
03:37:32.06 +64:51:18.5
03:39:34.54 +65:09:56.8
03:40:08.33 +65:14:33.3
05:56:21.20 +68:15:00.9
03:48:23.93 +65:27:30.8
03:41:00.67 +65:05:58.7
03:38:15.77 +65:04:36.2
03:45:13.76 +65:08:27.1
03:52:50.21 +64:55:48.6
03:41:04.42 +64:53:36.2
03:40:11.42 +64:52:55.7
03:34:04.39 +65:24:17.6
03:37:39.44 +65:22:17.8
04:55:33.07 +66:54:49.2
04:22:57.47 +71:18:48.8
04:33:22.65 +69:56:11.6
05:00:39.23 +69:23:42.2
05:03:01.60 +69:16:32.6
04:49:21.61 +64:57:31.3
04:38:05.77 +65:14:00.1
03:44:48.31 +65:16:41.2
03:41:04.90 +67:38:55.1
03:28:19.07 +68:29:58.4
04:05:39.59 +66:19:57.4
04:39:48.80 +66:23:44.0
########### 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 ####
03:39:14.87 +65:13:13.0
03:54:14.31 +65:06:44.3
03:35:50.78 +65:16:35.6
03:15:00.22 +70:30:11.4
03:36:12.01 +65:29:18.6
03:13:42.44 +71:37:45.0
03:44:54.11 +65:03:16.0
03:56:25.35 +65:16:19.9
03:56:58.17 +70:34:27.9
03:43:03.98 +68:35:28.1
04:32:14.46 +65:36:03.8
03:35:25.28 +67:46:27.5
03:19:57.13 +73:32:31.8
04:22:39.89 +68:29:26.3
03:41:15.95 +66:16:44.3
04:15:51.63 +65:54:40.4
03:28:48.37 +69:27:28.7
03:22:29.99 +70:00:50.4
03:23:14.61 +70:01:35.0
05:44:01.24 +68:13:19.6
03:32:19.85 +67:40:17.6
03:43:00.94 +66:17:03.1
05:10:02.21 +68:35:20.7
03:42:25.66 +64:48:24.0
03:19:32.15 +69:24:55.3
03:12:46.84 +73:28:15.2
03:43:46.25 +65:17:29.2
03:13:37.14 +70:50:51.2
03:24:41.48 +68:45:11.8
03:23:08.24 +69:38:53.2
03:13:11.66 +72:36:29.3
03:17:43.97 +72:32:06.5
03:22:54.84 +68:33:48.0
03:19:43.93 +69:27:22.1
03:21:05.38 +70:35:23.4
03:18:31.95 +71:59:23.6
03:27:41.45 +67:32:24.1
03:38:54.28 +65:23:50.6
03:11:44.36 +71:39:22.9
03:11:35.67 +71:41:32.4
05:02:20.34 +72:25:34.8
03:11:12.76 +71:36:40.6
03:36:18.86 +64:54:29.2
03:36:16.45 +64:54:22.5
04:51:34.01 +68:12:02.3
04:42:14.55 +69:04:10.5
03:11:06.49 +72:08:33.3
04:51:32.82 +68:11:46.1
03:17:24.50 +71:45:17.0
05:13:54.01 +67:29:16.7
04:18:40.76 +74:39:10.7
03:14:16.07 +70:32:08.8
03:30:00.25 +67:45:04.3
03:35:27.04 +65:32:13.9
03:19:36.54 +72:06:51.2
03:16:06.92 +72:04:22.5
04:57:37.86 +70:38:34.7
03:38:42.01 +65:20:21.7
03:16:27.35 +72:23:52.9
03:07:46.27 +72:53:43.2
04:02:57.94 +72:49:32.9
03:35:20.92 +65:32:13.2
05:20:28.75 +71:45:06.8
03:25:28.24 +67:58:18.1
03:41:10.31 +65:18:53.6
03:39:47.90 +64:48:07.8
03:35:48.57 +64:54:50.6
03:08:43.30 +72:37:12.3
05:58:41.51 +66:36:24.1
03:22:50.05 +73:24:19.5
04:47:21.97 +70:17:06.1
05:14:25.32 +69:50:42.1
03:11:51.22 +73:33:27.1
03:10:17.27 +72:32:36.5
03:15:50.18 +73:22:59.9
03:35:46.07 +64:54:43.9
03:27:15.02 +67:49:32.8
03:34:48.29 +65:06:05.0
03:37:59.67 +64:58:27.1
03:13:44.65 +72:20:21.0
05:19:27.02 +67:59:46.9
03:28:33.98 +67:12:39.8
03:36:51.56 +64:55:14.4
03:11:42.74 +72:13:51.7
05:22:35.24 +67:04:19.9
03:36:10.00 +65:20:47.6
03:35:47.81 +65:19:18.9
05:21:53.77 +67:02:52.9
03:15:44.05 +70:14:31.3
04:57:02.30 +71:52:52.4
05:15:53.73 +66:09:33.0
03:16:36.21 +71:35:41.8
03:53:46.25 +65:00:41.2
05:26:31.22 +70:13:21.3
03:25:19.25 +68:47:20.5
04:29:19.32 +69:15:32.8
05:17:16.00 +73:34:58.6
03:13:50.16 +71:48:22.4
03:37:57.02 +64:58:27.8
04:50:16.68 +72:56:17.1
03:57:57.19 +65:02:28.5
04:50:22.60 +72:53:50.0
03:16:54.08 +73:32:39.0
03:49:53.63 +64:58:42.9
05:46:33.73 +65:49:16.6
03:37:42.79 +64:57:11.5
03:05:57.14 +73:01:01.3
03:37:32.06 +64:51:18.5
03:39:34.54 +65:09:56.8
03:40:08.33 +65:14:33.3
05:56:21.20 +68:15:00.9
03:48:23.93 +65:27:30.8
03:41:00.67 +65:05:58.7
03:38:15.77 +65:04:36.2
03:45:13.76 +65:08:27.1
03:52:50.21 +64:55:48.6
03:41:04.42 +64:53:36.2
03:40:11.42 +64:52:55.7
03:34:04.39 +65:24:17.6
03:37:39.44 +65:22:17.8
04:55:33.07 +66:54:49.2
03:41:04.90 +67:38:55.1
04:38:05.77 +65:14:00.1
04:05:39.59 +66:19:57.4
05:03:14.32 +74:55:50.9
04:22:57.47 +71:18:48.8
05:03:01.60 +69:16:32.6
04:49:21.61 +64:57:31.3
05:00:39.23 +69:23:42.2
03:28:19.07 +68:29:58.4
04:39:48.80 +66:23:44.0
03:44:48.31 +65:16:41.2
04:33:22.65 +69:56:11.6
###################################################################################
03:39:14.87 +65:13:13.0 -- not an asteroid (will add it to exclusion list)
03:54:14.31 +65:06:44.3 -- not an asteroid (will add it to exclusion list)
03:35:50.78 +65:16:35.6 -- not an asteroid (will add it to exclusion list)
03:15:00.22 +70:30:11.4 -- not an asteroid (will add it to exclusion list)
03:36:12.01 +65:29:18.6 -- not an asteroid (will add it to exclusion list)
03:13:42.44 +71:37:45.0 -- not an asteroid (will add it to exclusion list)
03:44:54.11 +65:03:16.0 -- not an asteroid (will add it to exclusion list)
03:56:25.35 +65:16:19.9 -- not an asteroid (will add it to exclusion list)
03:56:58.17 +70:34:27.9 -- not an asteroid (will add it to exclusion list)
03:43:03.98 +68:35:28.1 -- not an asteroid (will add it to exclusion list)
04:32:14.46 +65:36:03.8 -- not an asteroid (will add it to exclusion list)
03:35:25.28 +67:46:27.5 -- not an asteroid (will add it to exclusion list)
03:19:57.13 +73:32:31.8 -- not an asteroid (will add it to exclusion list)
04:22:39.89 +68:29:26.3 -- not an asteroid (will add it to exclusion list)
03:41:15.95 +66:16:44.3 -- not an asteroid (will add it to exclusion list)
04:15:51.63 +65:54:40.4 -- not an asteroid (will add it to exclusion list)
03:28:48.37 +69:27:28.7 -- not an asteroid (will add it to exclusion list)
03:22:29.99 +70:00:50.4 -- not an asteroid (will add it to exclusion list)
03:23:14.61 +70:01:35.0 -- not an asteroid (will add it to exclusion list)
05:44:01.24 +68:13:19.6 -- not an asteroid (will add it to exclusion list)
03:32:19.85 +67:40:17.6 -- not an asteroid (will add it to exclusion list)
03:43:00.94 +66:17:03.1 -- not an asteroid (will add it to exclusion list)
05:10:02.21 +68:35:20.7 -- not an asteroid (will add it to exclusion list)
03:42:25.66 +64:48:24.0 -- not an asteroid (will add it to exclusion list)
03:19:32.15 +69:24:55.3 -- not an asteroid (will add it to exclusion list)
03:12:46.84 +73:28:15.2 -- not an asteroid (will add it to exclusion list)
03:43:46.25 +65:17:29.2 -- not an asteroid (will add it to exclusion list)
03:13:37.14 +70:50:51.2 -- not an asteroid (will add it to exclusion list)
03:24:41.48 +68:45:11.8 -- not an asteroid (will add it to exclusion list)
03:23:08.24 +69:38:53.2 -- not an asteroid (will add it to exclusion list)
03:13:11.66 +72:36:29.3 -- not an asteroid (will add it to exclusion list)
03:17:43.97 +72:32:06.5 -- not an asteroid (will add it to exclusion list)
03:22:54.84 +68:33:48.0 -- not an asteroid (will add it to exclusion list)
03:19:43.93 +69:27:22.1 -- not an asteroid (will add it to exclusion list)
03:21:05.38 +70:35:23.4 -- not an asteroid (will add it to exclusion list)
03:18:31.95 +71:59:23.6 -- not an asteroid (will add it to exclusion list)
03:27:41.45 +67:32:24.1 -- not an asteroid (will add it to exclusion list)
03:38:54.28 +65:23:50.6 -- not an asteroid (will add it to exclusion list)
03:11:44.36 +71:39:22.9 -- not an asteroid (will add it to exclusion list)
03:11:35.67 +71:41:32.4 -- not an asteroid (will add it to exclusion list)
05:02:20.34 +72:25:34.8 -- not an asteroid (will add it to exclusion list)
03:11:12.76 +71:36:40.6 -- not an asteroid (will add it to exclusion list)
03:36:18.86 +64:54:29.2 -- not an asteroid (will add it to exclusion list)
03:36:16.45 +64:54:22.5 -- not an asteroid (will add it to exclusion list)
04:51:34.01 +68:12:02.3 -- not an asteroid (will add it to exclusion list)
04:42:14.55 +69:04:10.5 -- not an asteroid (will add it to exclusion list)
03:11:06.49 +72:08:33.3 -- not an asteroid (will add it to exclusion list)
04:51:32.82 +68:11:46.1 -- not an asteroid (will add it to exclusion list)
03:17:24.50 +71:45:17.0 -- not an asteroid (will add it to exclusion list)
05:13:54.01 +67:29:16.7 -- not an asteroid (will add it to exclusion list)
04:18:40.76 +74:39:10.7 -- not an asteroid (will add it to exclusion list)
03:14:16.07 +70:32:08.8 -- not an asteroid (will add it to exclusion list)
03:30:00.25 +67:45:04.3 -- not an asteroid (will add it to exclusion list)
03:35:27.04 +65:32:13.9 -- not an asteroid (will add it to exclusion list)
03:19:36.54 +72:06:51.2 -- not an asteroid (will add it to exclusion list)
03:16:06.92 +72:04:22.5 -- not an asteroid (will add it to exclusion list)
04:57:37.86 +70:38:34.7 -- not an asteroid (will add it to exclusion list)
03:38:42.01 +65:20:21.7 -- not an asteroid (will add it to exclusion list)
03:16:27.35 +72:23:52.9 -- not an asteroid (will add it to exclusion list)
03:07:46.27 +72:53:43.2 -- not an asteroid (will add it to exclusion list)
04:02:57.94 +72:49:32.9 -- not an asteroid (will add it to exclusion list)
03:35:20.92 +65:32:13.2 -- not an asteroid (will add it to exclusion list)
05:20:28.75 +71:45:06.8 -- not an asteroid (will add it to exclusion list)
03:25:28.24 +67:58:18.1 -- not an asteroid (will add it to exclusion list)
03:41:10.31 +65:18:53.6 -- not an asteroid (will add it to exclusion list)
03:39:47.90 +64:48:07.8 -- not an asteroid (will add it to exclusion list)
03:35:48.57 +64:54:50.6 -- not an asteroid (will add it to exclusion list)
03:08:43.30 +72:37:12.3 -- not an asteroid (will add it to exclusion list)
05:58:41.51 +66:36:24.1 -- not an asteroid (will add it to exclusion list)
03:22:50.05 +73:24:19.5 -- not an asteroid (will add it to exclusion list)
04:47:21.97 +70:17:06.1 -- not an asteroid (will add it to exclusion list)
05:14:25.32 +69:50:42.1 -- not an asteroid (will add it to exclusion list)
03:11:51.22 +73:33:27.1 -- not an asteroid (will add it to exclusion list)
03:10:17.27 +72:32:36.5 -- not an asteroid (will add it to exclusion list)
03:15:50.18 +73:22:59.9 -- not an asteroid (will add it to exclusion list)
03:35:46.07 +64:54:43.9 -- not an asteroid (will add it to exclusion list)
03:27:15.02 +67:49:32.8 -- not an asteroid (will add it to exclusion list)
03:34:48.29 +65:06:05.0 -- not an asteroid (will add it to exclusion list)
03:37:59.67 +64:58:27.1 -- not an asteroid (will add it to exclusion list)
03:13:44.65 +72:20:21.0 -- not an asteroid (will add it to exclusion list)
05:19:27.02 +67:59:46.9 -- not an asteroid (will add it to exclusion list)
03:28:33.98 +67:12:39.8 -- not an asteroid (will add it to exclusion list)
03:36:51.56 +64:55:14.4 -- not an asteroid (will add it to exclusion list)
03:11:42.74 +72:13:51.7 -- not an asteroid (will add it to exclusion list)
05:22:35.24 +67:04:19.9 -- not an asteroid (will add it to exclusion list)
03:36:10.00 +65:20:47.6 -- not an asteroid (will add it to exclusion list)
03:35:47.81 +65:19:18.9 -- not an asteroid (will add it to exclusion list)
05:21:53.77 +67:02:52.9 -- not an asteroid (will add it to exclusion list)
03:15:44.05 +70:14:31.3 -- not an asteroid (will add it to exclusion list)
04:57:02.30 +71:52:52.4 -- not an asteroid (will add it to exclusion list)
05:15:53.73 +66:09:33.0 -- not an asteroid (will add it to exclusion list)
03:16:36.21 +71:35:41.8 -- not an asteroid (will add it to exclusion list)
03:53:46.25 +65:00:41.2 -- not an asteroid (will add it to exclusion list)
05:26:31.22 +70:13:21.3 -- not an asteroid (will add it to exclusion list)
03:25:19.25 +68:47:20.5 -- not an asteroid (will add it to exclusion list)
04:29:19.32 +69:15:32.8 -- not an asteroid (will add it to exclusion list)
05:17:16.00 +73:34:58.6 -- not an asteroid (will add it to exclusion list)
03:13:50.16 +71:48:22.4 -- not an asteroid (will add it to exclusion list)
03:37:57.02 +64:58:27.8 -- not an asteroid (will add it to exclusion list)
04:50:16.68 +72:56:17.1 -- not an asteroid (will add it to exclusion list)
03:57:57.19 +65:02:28.5 -- not an asteroid (will add it to exclusion list)
04:50:22.60 +72:53:50.0 -- not an asteroid (will add it to exclusion list)
03:16:54.08 +73:32:39.0 -- not an asteroid (will add it to exclusion list)
03:49:53.63 +64:58:42.9 -- not an asteroid (will add it to exclusion list)
05:46:33.73 +65:49:16.6 -- not an asteroid (will add it to exclusion list)
03:37:42.79 +64:57:11.5 -- not an asteroid (will add it to exclusion list)
03:05:57.14 +73:01:01.3 -- not an asteroid (will add it to exclusion list)
03:37:32.06 +64:51:18.5 -- not an asteroid (will add it to exclusion list)
03:39:34.54 +65:09:56.8 -- not an asteroid (will add it to exclusion list)
03:40:08.33 +65:14:33.3 -- not an asteroid (will add it to exclusion list)
05:56:21.20 +68:15:00.9 -- not an asteroid (will add it to exclusion list)
03:48:23.93 +65:27:30.8 -- not an asteroid (will add it to exclusion list)
03:41:00.67 +65:05:58.7 -- not an asteroid (will add it to exclusion list)
03:38:15.77 +65:04:36.2 -- not an asteroid (will add it to exclusion list)
03:45:13.76 +65:08:27.1 -- not an asteroid (will add it to exclusion list)
03:52:50.21 +64:55:48.6 -- not an asteroid (will add it to exclusion list)
03:41:04.42 +64:53:36.2 -- not an asteroid (will add it to exclusion list)
03:40:11.42 +64:52:55.7 -- not an asteroid (will add it to exclusion list)
03:34:04.39 +65:24:17.6 -- not an asteroid (will add it to exclusion list)
03:37:39.44 +65:22:17.8 -- not an asteroid (will add it to exclusion list)
04:55:33.07 +66:54:49.2 -- not an asteroid (will add it to exclusion list)
03:41:04.90 +67:38:55.1 -- not an asteroid (will add it to exclusion list)
04:38:05.77 +65:14:00.1 -- not an asteroid (will add it to exclusion list)
04:05:39.59 +66:19:57.4 -- not an asteroid (will add it to exclusion list)
05:03:14.32 +74:55:50.9 -- not an asteroid (will add it to exclusion list)
04:22:57.47 +71:18:48.8 -- not an asteroid (will add it to exclusion list)
05:03:01.60 +69:16:32.6 -- not an asteroid (will add it to exclusion list)
04:49:21.61 +64:57:31.3 -- not an asteroid (will add it to exclusion list)
05:00:39.23 +69:23:42.2 -- not an asteroid (will add it to exclusion list)
03:28:19.07 +68:29:58.4 -- not an asteroid (will add it to exclusion list)
04:39:48.80 +66:23:44.0 -- not an asteroid (will add it to exclusion list)
03:44:48.31 +65:16:41.2 -- not an asteroid (will add it to exclusion list)
04:33:22.65 +69:56:11.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:05:57.14 +73:01:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:46.27 +72:53:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:43.30 +72:37:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:10:17.27 +72:32:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:06.49 +72:08:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:12.76 +71:36:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:35.67 +71:41:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:42.74 +72:13:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:44.36 +71:39:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:11:51.22 +73:33:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:46.84 +73:28:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:11.66 +72:36:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:37.14 +70:50:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:42.44 +71:37:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:44.65 +72:20:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:50.16 +71:48:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:16.07 +70:32:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:00.22 +70:30:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:44.05 +70:14:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:50.18 +73:22:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:06.92 +72:04:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:27.35 +72:23:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:36.21 +71:35:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:16:54.08 +73:32:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:24.50 +71:45:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:43.97 +72:32:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:31.95 +71:59:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:32.15 +69:24:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:36.54 +72:06:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:43.93 +69:27:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:19:57.13 +73:32:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:05.38 +70:35:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:29.99 +70:00:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:50.05 +73:24:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:54.84 +68:33:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:08.24 +69:38:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:14.61 +70:01:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:41.48 +68:45:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:19.25 +68:47:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:28.24 +67:58:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:27:15.02 +67:49:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:27:41.45 +67:32:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:19.07 +68:29:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:33.98 +67:12:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:48.37 +69:27:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:00.25 +67:45:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:19.85 +67:40:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:04.39 +65:24:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:48.29 +65:06:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:20.92 +65:32:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:25.28 +67:46:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:27.04 +65:32:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:46.07 +64:54:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:47.81 +65:19:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:48.57 +64:54:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:50.78 +65:16:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:10.00 +65:20:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:12.01 +65:29:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:16.45 +64:54:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:18.86 +64:54:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:51.56 +64:55:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:32.06 +64:51:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:39.44 +65:22:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:42.79 +64:57:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:57.02 +64:58:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:59.67 +64:58:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:15.77 +65:04:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:42.01 +65:20:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:54.28 +65:23:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:14.87 +65:13:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:34.54 +65:09:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:47.90 +64:48:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:08.33 +65:14:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:11.42 +64:52:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:00.67 +65:05:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:04.42 +64:53:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:04.90 +67:38:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:10.31 +65:18:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:15.95 +66:16:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:25.66 +64:48:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:00.94 +66:17:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:03.98 +68:35:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:46.25 +65:17:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:48.31 +65:16:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:54.11 +65:03:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:13.76 +65:08:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:23.93 +65:27:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:53.63 +64:58:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:50.21 +64:55:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:46.25 +65:00:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:14.31 +65:06:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:25.35 +65:16:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:58.17 +70:34:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:57.19 +65:02:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:57.94 +72:49:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:39.59 +66:19:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:51.63 +65:54:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:40.76 +74:39:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:39.89 +68:29:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:57.47 +71:18:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:19.32 +69:15:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:14.46 +65:36:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:22.65 +69:56:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:05.77 +65:14:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:48.80 +66:23:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:14.55 +69:04:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:21.97 +70:17:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:21.61 +64:57:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:16.68 +72:56:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:22.60 +72:53:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:32.82 +68:11:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:34.01 +68:12:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:33.07 +66:54:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:02.30 +71:52:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:37.86 +70:38:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:39.23 +69:23:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:20.34 +72:25:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:01.60 +69:16:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:14.32 +74:55:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:02.21 +68:35:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:54.01 +67:29:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:25.32 +69:50:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:53.73 +66:09:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:16.00 +73:34:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:27.02 +67:59:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:28.75 +71:45:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:53.77 +67:02:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:35.24 +67:04:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:31.22 +70:13:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:01.24 +68:13:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:33.73 +65:49:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:21.20 +68:15:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:41.51 +66:36:24.1 -- 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)
03:05:57.14 +73:01:01.3 -- not a known variable star
03:07:46.27 +72:53:43.2 -- a known variable star
03:08:43.30 +72:37:12.3 -- not a known variable star
03:10:17.27 +72:32:36.5 -- a known variable star
03:11:06.49 +72:08:33.3 -- not a known variable star
03:11:12.76 +71:36:40.6 -- not a known variable star
03:11:35.67 +71:41:32.4 -- not a known variable star
03:11:42.74 +72:13:51.7 -- not a known variable star
03:11:44.36 +71:39:22.9 -- not a known variable star
03:11:51.22 +73:33:27.1 -- not a known variable star
03:12:46.84 +73:28:15.2 -- not a known variable star
03:13:11.66 +72:36:29.3 -- not a known variable star
03:13:37.14 +70:50:51.2 -- not a known variable star
03:13:42.44 +71:37:45.0 -- not a known variable star
03:13:44.65 +72:20:21.0 -- not a known variable star
03:13:50.16 +71:48:22.4 -- not a known variable star
03:14:16.07 +70:32:08.8 -- not a known variable star
03:15:00.22 +70:30:11.4 -- a known variable star
03:15:44.05 +70:14:31.3 -- not a known variable star
03:15:50.18 +73:22:59.9 -- not a known variable star
03:16:06.92 +72:04:22.5 -- not a known variable star
03:16:27.35 +72:23:52.9 -- not a known variable star
03:16:36.21 +71:35:41.8 -- not a known variable star
03:16:54.08 +73:32:39.0 -- not a known variable star
03:17:24.50 +71:45:17.0 -- not a known variable star
03:17:43.97 +72:32:06.5 -- not a known variable star
03:18:31.95 +71:59:23.6 -- not a known variable star
03:19:32.15 +69:24:55.3 -- not a known variable star
03:19:36.54 +72:06:51.2 -- not a known variable star
03:19:43.93 +69:27:22.1 -- not a known variable star
03:19:57.13 +73:32:31.8 -- not a known variable star
03:21:05.38 +70:35:23.4 -- not a known variable star
03:22:29.99 +70:00:50.4 -- not a known variable star
03:22:50.05 +73:24:19.5 -- a known variable star
03:22:54.84 +68:33:48.0 -- not a known variable star
03:23:08.24 +69:38:53.2 -- not a known variable star
03:23:14.61 +70:01:35.0 -- not a known variable star
03:24:41.48 +68:45:11.8 -- not a known variable star
03:25:19.25 +68:47:20.5 -- not a known variable star
03:25:28.24 +67:58:18.1 -- not a known variable star
03:27:15.02 +67:49:32.8 -- not a known variable star
03:27:41.45 +67:32:24.1 -- not a known variable star
03:28:19.07 +68:29:58.4 -- not a known variable star
03:28:33.98 +67:12:39.8 -- not a known variable star
03:28:48.37 +69:27:28.7 -- not a known variable star
03:30:00.25 +67:45:04.3 -- not a known variable star
03:32:19.85 +67:40:17.6 -- not a known variable star
03:34:04.39 +65:24:17.6 -- a known variable star
03:34:48.29 +65:06:05.0 -- not a known variable star
03:35:20.92 +65:32:13.2 -- not a known variable star
03:35:25.28 +67:46:27.5 -- not a known variable star
03:35:27.04 +65:32:13.9 -- not a known variable star
03:35:46.07 +64:54:43.9 -- not a known variable star
03:35:47.81 +65:19:18.9 -- not a known variable star
03:35:48.57 +64:54:50.6 -- not a known variable star
03:35:50.78 +65:16:35.6 -- not a known variable star
03:36:10.00 +65:20:47.6 -- not a known variable star
03:36:12.01 +65:29:18.6 -- not a known variable star
03:36:16.45 +64:54:22.5 -- a known variable star
03:36:18.86 +64:54:29.2 -- a known variable star
03:36:51.56 +64:55:14.4 -- a known variable star
03:37:32.06 +64:51:18.5 -- not a known variable star
03:37:39.44 +65:22:17.8 -- not a known variable star
03:37:42.79 +64:57:11.5 -- not a known variable star
03:37:57.02 +64:58:27.8 -- not a known variable star
03:37:59.67 +64:58:27.1 -- not a known variable star
03:38:15.77 +65:04:36.2 -- not a known variable star
03:38:42.01 +65:20:21.7 -- not a known variable star
03:38:54.28 +65:23:50.6 -- not a known variable star
03:39:14.87 +65:13:13.0 -- a known variable star
03:39:34.54 +65:09:56.8 -- not a known variable star
03:39:47.90 +64:48:07.8 -- not a known variable star
03:40:08.33 +65:14:33.3 -- not a known variable star
03:40:11.42 +64:52:55.7 -- not a known variable star
03:41:00.67 +65:05:58.7 -- not a known variable star
03:41:04.42 +64:53:36.2 -- not a known variable star
03:41:04.90 +67:38:55.1 -- a known variable star
03:41:10.31 +65:18:53.6 -- not a known variable star
03:41:15.95 +66:16:44.3 -- not a known variable star
03:42:25.66 +64:48:24.0 -- not a known variable star
03:43:00.94 +66:17:03.1 -- not a known variable star
03:43:03.98 +68:35:28.1 -- a known variable star
03:43:46.25 +65:17:29.2 -- not a known variable star
03:44:48.31 +65:16:41.2 -- not a known variable star
03:44:54.11 +65:03:16.0 -- not a known variable star
03:45:13.76 +65:08:27.1 -- a known variable star
03:48:23.93 +65:27:30.8 -- not a known variable star
03:49:53.63 +64:58:42.9 -- not a known variable star
03:52:50.21 +64:55:48.6 -- not a known variable star
03:53:46.25 +65:00:41.2 -- not a known variable star
03:54:14.31 +65:06:44.3 -- not a known variable star
03:56:25.35 +65:16:19.9 -- a known variable star
03:56:58.17 +70:34:27.9 -- a known variable star
03:57:57.19 +65:02:28.5 -- a known variable star
04:02:57.94 +72:49:32.9 -- not a known variable star
04:05:39.59 +66:19:57.4 -- a known variable star
04:15:51.63 +65:54:40.4 -- not a known variable star
04:18:40.76 +74:39:10.7 -- not a known variable star
04:22:39.89 +68:29:26.3 -- not a known variable star
04:22:57.47 +71:18:48.8 -- a known variable star
04:29:19.32 +69:15:32.8 -- not a known variable star
04:32:14.46 +65:36:03.8 -- a known variable star
04:33:22.65 +69:56:11.6 -- a known variable star
04:38:05.77 +65:14:00.1 -- a known variable star
04:39:48.80 +66:23:44.0 -- a known variable star
04:42:14.55 +69:04:10.5 -- not a known variable star
04:47:21.97 +70:17:06.1 -- not a known variable star
04:49:21.61 +64:57:31.3 -- a known variable star
04:50:16.68 +72:56:17.1 -- not a known variable star
04:50:22.60 +72:53:50.0 -- not a known variable star
04:51:32.82 +68:11:46.1 -- not a known variable star
04:51:34.01 +68:12:02.3 -- not a known variable star
04:55:33.07 +66:54:49.2 -- not a known variable star
04:57:02.30 +71:52:52.4 -- not a known variable star
04:57:37.86 +70:38:34.7 -- not a known variable star
05:00:39.23 +69:23:42.2 -- not a known variable star
05:02:20.34 +72:25:34.8 -- not a known variable star
05:03:01.60 +69:16:32.6 -- a known variable star
05:03:14.32 +74:55:50.9 -- not a known variable star
05:10:02.21 +68:35:20.7 -- not a known variable star
05:13:54.01 +67:29:16.7 -- not a known variable star
05:14:25.32 +69:50:42.1 -- not a known variable star
05:15:53.73 +66:09:33.0 -- not a known variable star
05:17:16.00 +73:34:58.6 -- not a known variable star
05:19:27.02 +67:59:46.9 -- not a known variable star
05:20:28.75 +71:45:06.8 -- not a known variable star
05:21:53.77 +67:02:52.9 -- not a known variable star
05:22:35.24 +67:04:19.9 -- a known variable star
05:26:31.22 +70:13:21.3 -- not a known variable star
05:44:01.24 +68:13:19.6 -- a known variable star
05:46:33.73 +65:49:16.6 -- not a known variable star
05:56:21.20 +68:15:00.9 -- not a known variable star
05:58:41.51 +66:36:24.1 -- not a known variable star
Found 108 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
133 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)2461083.99765101 -observatory 500
22:43:17.37 -08:36:26.1 Mercury (-1.1mag)
22:18:58.29 -12:02:48.9 Venus (-3.9mag)
21:12:42.06 -17:14:54.4 Mars (1.1mag)
07:08:59.99 +22:48:53.1 Jupiter (-2.6mag)
00:01:28.30 -02:11:08.6 Saturn (1.0mag)
03:39:31.78 +19:20:00.5 Uranus (5.7mag)
00:02:30.55 -01:09:25.5 Neptune (7.8mag)
20:27:53.42 -23:02:31.9 Pluto (14.6mag)
17:40:37.68 -28:23:31.8 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Feb 12 06:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461083.99765101:
07:08:51.71 +22:49:06.7 Io (5.3mag)
07:09:04.74 +22:48:39.2 Europa (5.5mag)
07:08:45.88 +22:49:12.8 Ganymede (4.9mag)
07:08:59.89 +22:48:40.5 Callisto (6.0mag)
07:11:18.08 +23:09:07.7 Himalia (15.0mag)
07:08:53.87 +22:49:04.0 Thebe (15.8mag)
07:10:55.14 +23:11:59.7 Elara (17.0mag)
07:04:06.48 +24:01:51.4 Pasiphae (17.0mag)
07:18:01.09 +22:33:51.0 Carme (18.0mag)
00:01:22.85 -02:10:48.2 Titan (8.7mag)
00:01:30.97 -02:11:06.4 Rhea (10.1mag)
00:01:03.79 -02:12:52.3 Iapetus (11.5mag)
00:01:30.20 -02:10:53.6 Hyperion (14.7mag)
00:03:34.21 -01:57:44.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 12 06:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461083.99765101:
07:41:38.86 +23:00:23.5 JWST
17:17:33.25 +42:16:21.7 Chandra
18:25:36.50 -16:38:24.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 12 06:00 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)2461083.99765101 at 500
16:41:05.96 -10:51:40.4 17.7mag 10P/Tempel
03:29:05.36 +28:26:35.6 18.1mag 123P/West-Hartley
20:48:42.77 -10:07:01.3 22.4mag 141P/Machholz
01:00:04.99 +09:08:45.5 17.6mag 145P/Shoemaker-Levy 5
11:11:48.90 +29:19:16.4 17.8mag 164P/Christensen
09:38:39.35 -34:07:38.2 18.0mag 195P/Hill
15:51:04.60 -07:24:36.8 18.5mag 210P/Christensen
17:31:21.09 -21:38:46.0 17.4mag 218P/LINEAR
16:04:21.11 -18:17:31.5 15.2mag 235P/LINEAR
03:43:37.55 +25:53:45.3 17.5mag 240P/NEAT
15:03:12.66 +07:29:01.6 14.6mag 24P/Schaumasse
23:54:44.11 +04:21:34.1 18.1mag 261P/Larson
11:27:11.33 -03:35:33.1 17.4mag 29P/Schwassmann-Wachmann 1
01:07:26.49 +01:27:21.8 18.9mag 302P/Lemmon-PanSTARRS
07:06:33.13 +27:17:28.1 19.7mag 407P/PanSTARRS-Fuls
16:50:13.95 -11:18:47.1 17.5mag 40P/Vaisala 1
11:08:03.24 -09:15:37.6 16.6mag 43P/Wolf-Harrington
13:22:55.58 -05:09:06.1 19.4mag 489P/Denning
04:28:09.60 +49:23:33.6 17.7mag 493P/2024 Q2 (LONEOS)
06:02:39.12 +49:15:25.9 17.8mag 63P/Wild 1
22:55:35.81 -03:51:11.1 16.3mag 78P/Gehrels 2
19:25:11.76 -23:27:39.7 15.1mag 88P/Howell
15:22:12.24 -28:11:52.4 18.7mag P/2023 S1 (PanSTARRS)
04:43:14.67 -73:08:27.3 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:37.29 +31:11:11.1 18.1mag C/2017 K2 (PanSTARRS)
20:00:57.15 -64:56:32.2 18.1mag C/2020 V2 (ZTF)
17:17:12.46 +03:23:07.0 16.3mag C/2021 G2 (ATLAS)
22:45:54.01 +28:36:17.5 16.8mag C/2022 E2 (ATLAS)
03:28:28.94 +24:26:45.6 15.7mag C/2022 N2 (PANSTARRS)
09:11:46.57 +28:58:47.3 15.3mag C/2022 QE78 (ATLAS)
08:38:51.32 -07:42:57.6 16.6mag C/2022 R6 (PanSTARRS)
23:40:59.21 +48:06:59.2 17.9mag C/2023 C2 (ATLAS)
10:01:55.43 -22:03:56.4 17.5mag C/2023 F3 (ATLAS)
20:14:31.96 +61:17:07.8 17.2mag C/2023 H5 (Lemmon)
19:32:57.82 -03:17:55.5 16.1mag C/2023 R1 (PANSTARRS)
02:46:00.88 +35:46:59.3 18.5mag C/2023 RS61 (PanSTARRS)
20:43:59.70 +81:15:28.7 18.0mag C/2023 X2 (Lemmon)
06:55:02.85 +63:26:13.5 17.2mag C/2024 A1 (ATLAS)
00:33:04.15 -36:38:03.3 10.8mag C/2024 E1 (Wierzchos)
11:52:13.57 -04:20:20.8 18.1mag C/2024 G2 (ATLAS)
19:18:49.81 +00:21:38.5 19.0mag C/2024 G4 (PanSTARRS)
16:36:59.84 -02:55:00.0 17.8mag C/2024 G6 (ATLAS)
19:46:38.72 +01:33:26.5 15.6mag C/2024 J3 (ATLAS)
02:42:36.80 -33:24:26.1 15.4mag C/2024 T5 (ATLAS)
16:45:59.44 -54:26:52.9 15.3mag C/2025 A6 (Lemmon)
04:55:01.78 +66:08:06.6 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)
16:01:06.76 -20:02:30.1 15.0mag C/2025 L1 (ATLAS)
02:12:50.28 -17:39:31.3 16.7mag C/2025 Q3 (ATLAS)
01:57:12.30 +16:20:49.4 20.8mag C/2025 R2 (SWAN)
22:17:30.97 +17:32:35.7 16.8mag C/2025 R3 (PANSTARRS)
21:35:28.94 -14:44:10.5 20.4mag C/2025 T1 (ATLAS)
03:30:26.99 -25:02:29.0 17.4mag C/2026 A1 (MAPS)
20:26:45.04 +16:22:08.3 16.6mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.7K Feb 12 06:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
18:16:39.86 -19:51:57.30 TCP J06282145-1950371 2026-02-9.38 15.25
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
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
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
07:40:22.22 -10:00:59.30 AT2025aftz 2025-12-8.46 15.46
18:44:55.93 +47:57:37.60 ASASSN-25ez 2025-12-3.07 15.16
22:41:03.48 +38:58:01.90 ASASSN-25ey 2025-11-26.08 15.68
05:50:46.62 +58:54:53.50 SN 2025aedz 2025-11-24.25 16.66
06:35:50.19 -71:30:42.00 SN 2025adwn 2025-11-24.11 17.58
02:21:35.59 -14:18:04.90 AT2025aeft 2025-11-23.13 16.82
01:42:47.75 +12:31:45.10 AT2025aduf 2025-11-23.15 17.49
-rw-r--r-- 1 apache apache 6.2K Feb 12 06:00 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:28.44 +41:18:24.5 TCP J00422844+4118245 2025-12-22.8736 18.5mag
16:42:59.22 +26:21:02.0 TCP J16425922+2621020 2025-12-26.8538 13.0mag
08:08:08.72 -19:48:46.5 TCP J08080872-1948465 2025-12-27.7904 16.66Cmag
00:42:58.48 +41:08:11.4 PNV J00425848+4108114 2025-12-28.7654 18.9mag
07:35:31.47 +09:10:34.1 TCP J07353147+0910341 2025-12-29.7527 14.77Cmag
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
-rw-r--r-- 1 apache apache 186K Feb 12 06:00 tocp_transients_list.txt
