This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.27 05:56:34.37 +59:18:10.5
154.08296 16.52063 galactic Cam Second-epoch detections are separated by 6.3" and 7.6 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 269922068736669312 | 05:56:35.69 +59:18:15.0 (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 269922068736669312,2461083.9934,11.27,0.05,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 269922068736669312 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:34.37 +59:18:10.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.20 05:53:18.26 +61:26:49.6
151.88112 17.08420 galactic Cam Second-epoch detections are separated by 3.4" and 7.3 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 283313845486348416 | 05:53:19.60 +61:26:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 283313845486348416,2461083.9934,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 283313845486348416 20260212.4934 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:18.26 +61:26:49.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.14 05:52:29.33 +63:09:38.1
150.21773 17.73679 galactic Cam Second-epoch detections are separated by 3.6" and 6.6 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 286707178888012800 | 05:52:28.28 +63:09:38.3 (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 286707178888012800,2461083.9934,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286707178888012800 20260212.4934 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:29.33 +63:09:38.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.74 05:58:18.38 +57:54:01.6
155.50240 16.11792 galactic Cam Second-epoch detections are separated by 1.3" and 7.1 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 268801387214851328 | 05:58:17.73 +57:53:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 268801387214851328,2461083.9934,10.74,0.05,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 268801387214851328 20260212.4934 10.74CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:18.38 +57:54:01.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.61 05:52:42.43 +60:44:34.8
152.51062 16.71246 galactic Cam Second-epoch detections are separated by 3.4" and 6.2 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 282468458484327424 | 05:52:44.22 +60:44:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+60 491
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 282468458484327424,2461083.9934,10.61,0.05,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 282468458484327424 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:42.43 +60:44:34.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.42 05:42:49.25 +64:06:54.4
148.82304 17.19586 galactic Cam Second-epoch detections are separated by 3.5" and 6.4 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 287747488686097664 | 05:42:50.78 +64:06:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+64 321
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 287747488686097664,2461083.9934,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287747488686097664 20260212.4934 10.42CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:49.25 +64:06:54.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.63 05:48:25.58 +63:43:14.4
149.48147 17.57046 galactic Cam Second-epoch detections are separated by 3.2" and 7.1 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 286938041970400640 | 05:48:27.10 +63:43:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+63 385
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 286938041970400640,2461083.9934,10.63,0.05,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 286938041970400640 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:25.58 +63:43:14.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.78 05:49:45.58 +65:56:14.3
147.44216 18.65532 galactic Cam Second-epoch detections are separated by 1.5" and 6.6 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 | Large-amplitude variable Gaia DR2 480343442963819648 | 05:49:47.34 +65:56:10.1 (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) SpType: G5 1956PMcCO..13a....B AG+65 324
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480343442963819648,2461083.9934,10.78,0.05,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
Large-amplitude variable Gaia DR2 480343442963819648 20260212.4934 10.78CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:45.58 +65:56:14.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 2234660,2461083.9934,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2234660 20260212.4934 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:30.30 +63:19:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.14 05:55:56.65 +64:29:48.6
149.10909 18.64308 galactic Cam Second-epoch detections are separated by 7.3" and 8.1 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 287087884786612608 | 05:55:57.92 +64:29:46.7 (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 287087884786612608,2461083.9934,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287087884786612608 20260212.4934 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:56.65 +64:29:48.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.27 05:56:48.35 +66:15:45.9
147.43909 19.43965 galactic Cam Second-epoch detections are separated by 4.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 480375294441356288 | 05:56:49.66 +66:15:42.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480375294441356288,2461083.9934,11.27,0.05,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
Large-amplitude variable Gaia DR2 480375294441356288 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:48.35 +66:15:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.49 05:46:30.08 +64:46:41.0
148.38808 17.84774 galactic Cam Second-epoch detections are separated by 1.3" and 6.9 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 287987216580527360 | 05:46:31.06 +64:46:41.3 (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 287987216580527360,2461083.9934,11.49,0.05,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
Gaia DR3 287987216580527360 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:30.08 +64:46:41.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
KR Cam,2461083.9934,10.65,0.05,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
KR Cam 20260212.4934 10.65CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:02.69 +59:32:22.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
U Lyn,2461083.9934,10.13,0.05,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
U Lyn 20260212.4934 10.13CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:46.74 +59:52:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
VARIABLE_NAME,2461083.9934,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.4934 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:04.96 +58:29:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.27 05:57:09.07 +57:09:59.9
156.11886 15.65861 galactic Cam Second-epoch detections are separated by 4.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.2880+57.1685 | 05:57:09.12 +57:10:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J089.2880+57.1685,2461083.9934,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2880+57.1685 20260212.4934 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:09.07 +57:09:59.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.35 05:49:59.24 +64:14:24.6
149.06861 17.95072 galactic Cam Second-epoch detections are separated by 3.9" and 6.6 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 287808271063686784 | 05:50:00.02 +64:14:18.9 (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 287808271063686784,2461083.9934,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287808271063686784 20260212.4934 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:59.24 +64:14:24.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.29 05:53:06.27 +59:24:32.4
153.78215 16.16956 galactic Cam Second-epoch detections are separated by 6.4" 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 270100357123640960 | 05:53:07.01 +59:24:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 270100357123640960,2461083.9934,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 270100357123640960 20260212.4934 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:06.27 +59:24:32.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.22 05:51:47.53 +59:52:00.9
153.27819 16.22405 galactic Cam Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 282183959849705856 | 05:51:48.33 +59:52:02.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 282183959849705856,2461083.9934,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 282183959849705856 20260212.4934 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:47.53 +59:52:00.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.35 05:52:17.47 +60:03:51.8
153.12264 16.36759 galactic Cam Second-epoch detections are separated by 3.5" and 7.1 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 282199902768474624 | 05:52:17.55 +60:03:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 282199902768474624,2461083.9934,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282199902768474624 20260212.4934 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:17.47 +60:03:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.17 06:05:32.40 +57:59:30.5
155.83770 17.02684 galactic Cam Second-epoch detections are separated by 1.0" and 6.8 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 999125735124738560 | 06:05:33.04 +57:59:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 999125735124738560,2461083.9934,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 999125735124738560 20260212.4934 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:32.40 +57:59:30.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.07 06:02:27.28 +57:35:01.1
156.04703 16.48327 galactic Cam Second-epoch detections are separated by 7.2" and 7.3 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 999065880459478528 | 06:02:27.96 +57:35:05.7 (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 999065880459478528,2461083.9934,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 999065880459478528 20260212.4934 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:27.28 +57:35:01.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.23 05:53:30.54 +65:20:10.2
148.18950 18.75421 galactic Cam Second-epoch detections are separated by 7.3" and 6.4 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 | 05:53:30.54 +65:20:10.2 (user input) | T | P | (position from user input) J-Ks=0.261+/-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,2461083.9934,13.23,0.05,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
target 20260212.4934 13.23CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:30.54 +65:20:10.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.04 05:56:36.66 +59:10:44.8
154.20160 16.47151 galactic Cam Second-epoch detections are separated by 4.1" and 7.0 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 269905777925407104 | 05:56:37.36 +59:10:47.9 (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 269905777925407104,2461083.9934,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 269905777925407104 20260212.4934 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:36.66 +59:10:44.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.18 06:06:55.09 +66:06:35.7
148.00346 20.32479 galactic Cam Second-epoch detections are separated by 8.3" and 6.6 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 1104810689707144448 | 06:06:56.07 +66:06:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1104810689707144448,2461083.9934,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1104810689707144448 20260212.4934 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:55.09 +66:06:35.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.17 06:10:57.32 +60:41:12.7
153.52261 18.72538 galactic Cam Second-epoch detections are separated by 4.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:10:57.32 +60:41:12.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461083.9934,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:57.32 +60:41:12.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.92 05:58:55.34 +60:24:53.8
153.16282 17.26117 galactic Cam Second-epoch detections are separated by 5.8" and 7.6 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 | ATO J089.7453+60.4118 | 05:58:54.68 +60:24:59.8 (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 J089.7453+60.4118,2461083.9934,12.92,0.05,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
ATO J089.7453+60.4118 20260212.4934 12.92CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:55.34 +60:24:53.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 282317889813879552,2461083.9934,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282317889813879552 20260212.4934 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:46.47 +61:04:53.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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,2461083.9934,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:47.33 +64:03:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.81 05:52:04.84 +58:38:05.8
154.44176 15.70670 galactic Cam Second-epoch detections are separated by 5.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.0009+58.6330 | 05:52:04.05 +58:37:58.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J088.0009+58.6330,2461083.9934,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.0009+58.6330 20260212.4934 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:04.84 +58:38:05.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.65 06:10:06.93 +57:10:09.0
156.88457 17.25490 galactic Cam Second-epoch detections are separated by 3.0" and 7.2 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 | Large-amplitude variable Gaia DR2 998807911840016768 | 06:10:06.27 +57:10:05.5 (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) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 998807911840016768,2461083.9934,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 998807911840016768 20260212.4934 12.65CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:06.93 +57:10:09.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.72 05:49:20.22 +62:43:51.2
150.46031 17.22735 galactic Cam Second-epoch detections are separated by 7.9" and 7.1 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 286592211203611264 | 05:49:18.61 +62:43:51.6 (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 286592211203611264,2461083.9934,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286592211203611264 20260212.4934 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:20.22 +62:43:51.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.62 05:50:15.91 +61:27:35.6
151.70285 16.76341 galactic Cam Second-epoch detections are separated by 7.7" and 7.2 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 283232653424996864 | 05:50:15.06 +61:27:36.3 (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 283232653424996864,2461083.9934,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 283232653424996864 20260212.4934 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:15.91 +61:27:35.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.62 05:50:16.33 +63:20:32.3
149.93275 17.59019 galactic Cam Second-epoch detections are separated by 4.3" and 7.0 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 286771431598782464 | 05:50:15.24 +63:20:34.2 (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 286771431598782464,2461083.9934,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286771431598782464 20260212.4934 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:16.33 +63:20:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.65 05:56:13.16 +64:32:17.8
149.08200 18.68707 galactic Cam Second-epoch detections are separated by 5.4" and 6.3 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 287090186891246848 | 05:56:14.43 +64:32:16.6 (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 287090186891246848,2461083.9934,12.65,0.05,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
Gaia DR3 287090186891246848 20260212.4934 12.65CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:13.16 +64:32:17.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 2209083,2461083.9934,12.36,0.05,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
NSVS 2209083 20260212.4934 12.36CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:06.93 +60:10:40.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 269857369349492992,2461083.9934,12.23,0.05,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 269857369349492992 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:34.70 +59:04:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.35 05:52:38.74 +58:36:48.2
154.49601 15.76280 galactic Cam Second-epoch detections are separated by 2.2" and 7.2 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 269819126961380608 | 05:52:37.83 +58:36:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 269819126961380608,2461083.9934,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 269819126961380608 20260212.4934 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:38.74 +58:36:48.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.11 05:48:08.13 +60:41:41.2
152.29598 16.19053 galactic Cam Second-epoch detections are separated by 3.1" and 6.7 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 282432174599650048 | 05:48:07.40 +60:41:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 282432174599650048,2461083.9934,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 282432174599650048 20260212.4934 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:08.13 +60:41:41.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.07 06:03:52.87 +57:16:15.7
156.42701 16.52639 galactic Cam Second-epoch detections are separated by 3.1" and 7.0 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 | ATO J090.9841+57.2687 | 06:03:53.90 +57:16:25.9 (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 J090.9841+57.2687,2461083.9934,12.07,0.05,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
ATO J090.9841+57.2687 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:52.87 +57:16:15.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.70 05:56:41.98 +59:24:23.7
153.99269 16.57996 galactic Cam Second-epoch detections are separated by 6.1" and 7.8 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 270111214799985920 | 05:56:43.55 +59:24:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 270111214799985920,2461083.9934,11.70,0.05,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 270111214799985920 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:41.98 +59:24:23.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 10.68 05:46:40.91 +65:49:25.3
147.40785 18.32258 galactic Cam Second-epoch detections are separated by 0.7" and 6.8 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 480262422702056832 | 05:46:42.09 +65:49:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B AG+65 321
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480262422702056832,2461083.9934,10.68,0.05,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 480262422702056832 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:40.91 +65:49:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.37 05:47:09.37 +65:06:35.0
148.10677 18.05556 galactic Cam Second-epoch detections are separated by 0.6" and 6.8 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 288015288486521856 | 05:47:10.60 +65:06:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B AG+65 322
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 288015288486521856,2461083.9934,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 288015288486521856 20260212.4934 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:09.37 +65:06:35.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.37 05:41:01.02 +64:55:13.4
147.97996 17.39112 galactic Cam Second-epoch detections are separated by 1.7" and 7.0 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 288039649541160960 | 05:41:02.33 +64:55:13.2 (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 288039649541160960,2461083.9934,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 288039649541160960 20260212.4934 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:01.02 +64:55:13.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.33 05:52:26.91 +63:09:39.7
150.21526 17.73287 galactic Cam Second-epoch detections are separated by 2.5" and 6.8 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 286707178888012800 | 05:52:28.28 +63:09:38.3 (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 286707178888012800,2461083.9934,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 286707178888012800 20260212.4934 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:26.91 +63:09:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.54 05:47:43.75 +65:06:43.1
148.13229 18.11080 galactic Cam Second-epoch detections are separated by 0.7" and 6.7 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 288012604130323456 | 05:47:45.00 +65:06:41.2 (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 288012604130323456,2461083.9934,11.54,0.05,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 288012604130323456 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:43.75 +65:06:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.61 05:48:53.22 +63:58:13.1
149.26925 17.72538 galactic Cam Second-epoch detections are separated by 4.7" and 5.9 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 286957558301758720 | 05:48:55.07 +63:58:12.7 (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 286957558301758720,2461083.9934,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286957558301758720 20260212.4934 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.22 +63:58:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.71 05:58:16.10 +65:30:13.1
148.24021 19.27449 galactic Cam Second-epoch detections are separated by 4.4" and 6.5 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 287945160260946560 | 05:58:17.70 +65:30:09.5 (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 287945160260946560,2461083.9934,11.71,0.05,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 287945160260946560 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:16.10 +65:30:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.71 05:54:14.98 +65:04:06.9
148.48066 18.71413 galactic Cam Second-epoch detections are separated by 1.5" and 6.9 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 287895613518275456 | 05:54:16.38 +65:04:02.0 (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 287895613518275456,2461083.9934,11.71,0.05,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 287895613518275456 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:14.98 +65:04:06.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.53 05:55:23.95 +58:00:33.0
155.22548 15.81851 galactic Cam Second-epoch detections are separated by 2.0" and 6.6 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 | ATO J088.8618+58.0056 | 05:55:23.21 +58:00:28.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J088.8618+58.0056,2461083.9934,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.8618+58.0056 20260212.4934 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:23.95 +58:00:33.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.84 05:56:29.09 +66:29:22.0
147.20498 19.50052 galactic Cam Second-epoch detections are separated by 2.6" and 7.0 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 480394016202970624 | 05:56:30.54 +66:29:19.8 (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 480394016202970624,2461083.9934,11.84,0.05,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 480394016202970624 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:29.09 +66:29:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.87 05:52:53.12 +65:20:49.6
148.15045 18.69959 galactic Cam Second-epoch detections are separated by 1.5" and 7.1 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 288104520728279936 | 05:52:54.50 +65:20:47.3 (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 288104520728279936,2461083.9934,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 288104520728279936 20260212.4934 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:53.12 +65:20:49.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.84 05:55:47.91 +64:54:56.9
148.69881 18.80054 galactic Cam Second-epoch detections are separated by 1.9" and 6.8 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 287863006126726528 | 05:55:49.49 +64:54:53.9 (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 287863006126726528,2461083.9934,11.84,0.05,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 287863006126726528 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:47.91 +64:54:56.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.83 05:52:10.92 +64:17:55.7
149.12004 18.19110 galactic Cam Second-epoch detections are separated by 0.2" and 6.7 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 287059022608456960 | 05:52:12.72 +64:17:52.4 (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 287059022608456960,2461083.9934,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 287059022608456960 20260212.4934 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:10.92 +64:17:55.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.93 05:54:35.49 +66:18:21.9
147.30210 19.25325 galactic Cam Second-epoch detections are separated by 4.0" and 7.1 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 480390137850745088 | 05:54:37.42 +66:18:17.1 (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 480390137850745088,2461083.9934,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480390137850745088 20260212.4934 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:35.49 +66:18:21.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.03 05:56:04.10 +65:55:08.6
147.74105 19.23344 galactic Cam Second-epoch detections are separated by 4.4" and 6.7 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 288201896226549888 | 05:56:05.95 +65:55:06.2 (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 288201896226549888,2461083.9934,12.03,0.05,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 288201896226549888 20260212.4934 12.03CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:04.10 +65:55:08.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.14 05:54:49.11 +66:31:53.0
147.09357 19.36527 galactic Cam Second-epoch detections are separated by 4.2" and 6.8 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 480443842120827136 | 05:54:50.21 +66:31:50.6 (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 480443842120827136,2461083.9934,12.14,0.05,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 480443842120827136 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:49.11 +66:31:53.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.96 05:57:26.87 +57:25:23.9
155.89738 15.80707 galactic Cam Second-epoch detections are separated by 6.5" and 7.2 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 268724180881521408 | 05:57:26.28 +57:25:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 268724180881521408,2461083.9934,11.96,0.05,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 268724180881521408 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:26.87 +57:25:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.12 05:48:53.92 +65:58:49.5
147.36161 18.59432 galactic Cam Second-epoch detections are separated by 1.7" and 6.6 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 480265205841548672 | 05:48:55.42 +65:58:49.3 (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 480265205841548672,2461083.9934,12.12,0.05,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 480265205841548672 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.92 +65:58:49.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.13 05:53:19.26 +66:17:40.9
147.25793 19.13206 galactic Cam Second-epoch detections are separated by 5.9" and 6.2 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 480370140482078848 | 05:53:21.06 +66:17:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 480370140482078848,2461083.9934,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480370140482078848 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:19.26 +66:17:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 480366463990069888,2461083.9934,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480366463990069888 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:48.84 +66:15:04.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.19 05:50:05.51 +66:07:57.6
147.27036 18.76856 galactic Cam Second-epoch detections are separated by 0.6" and 6.8 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 480361138230696832 | 05:50:07.03 +66:07:58.0 (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 480361138230696832,2461083.9934,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480361138230696832 20260212.4934 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:05.51 +66:07:57.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.15 05:53:57.43 +64:35:48.4
148.91996 18.49004 galactic Cam Second-epoch detections are separated by 2.5" and 6.6 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 287820709288873216 | 05:53:59.01 +64:35:47.2 (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 287820709288873216,2461083.9934,12.15,0.05,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 287820709288873216 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:57.43 +64:35:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
ZTF J055030.00+641555.2,2461083.9934,12.15,0.05,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
ZTF J055030.00+641555.2 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:32.44 +64:16:13.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.18 05:46:04.73 +65:59:45.4
147.21628 18.34226 galactic Cam Second-epoch detections are separated by 1.3" and 6.7 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 480309461184581120 | 05:46:05.87 +65:59:43.5 (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 480309461184581120,2461083.9934,12.18,0.05,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 480309461184581120 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:04.73 +65:59:45.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 11.98 05:57:16.53 +63:54:56.9
149.73090 18.53717 galactic Cam Second-epoch detections are separated by 7.0" and 7.5 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 286812697644361088 | 05:57:17.43 +63:54:56.4 (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 286812697644361088,2461083.9934,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286812697644361088 20260212.4934 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:16.53 +63:54:56.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.14 05:54:49.56 +63:46:24.3
149.74997 18.23252 galactic Cam Second-epoch detections are separated by 5.0" and 6.0 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 286787443236721152 | 05:54:50.94 +63:46:21.2 (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 286787443236721152,2461083.9934,12.14,0.05,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 286787443236721152 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:49.56 +63:46:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.20 05:45:56.54 +65:07:38.0
148.03131 17.94852 galactic Cam Second-epoch detections are separated by 0.2" and 6.9 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 288057173007611648 | 05:45:58.22 +65:07:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+65 319
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 288057173007611648,2461083.9934,12.20,0.05,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 288057173007611648 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:56.54 +65:07:38.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.10 05:54:39.86 +61:58:47.2
151.45000 17.45866 galactic Cam Second-epoch detections are separated by 3.4" and 6.4 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 283387856362590080 | 05:54:41.05 +61:58:46.2 (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 283387856362590080,2461083.9934,12.10,0.05,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
Gaia DR3 283387856362590080 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:39.86 +61:58:47.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.10 05:56:01.74 +57:22:49.0
155.85032 15.61650 galactic Cam Second-epoch detections are separated by 4.5" and 7.6 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 268726208106090496 | 05:56:00.82 +57:22:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 268726208106090496,2461083.9934,12.10,0.05,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
Gaia DR3 268726208106090496 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:01.74 +57:22:49.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.15 05:52:44.53 +63:42:44.0
149.70621 17.99772 galactic Cam Second-epoch detections are separated by 6.4" and 7.3 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 286973771801312640 | 05:52:45.46 +63:42:43.7 (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 286973771801312640,2461083.9934,12.15,0.05,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 286973771801312640 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:44.53 +63:42:44.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.19 06:04:50.55 +66:41:30.9
147.34477 20.34476 galactic Cam Second-epoch detections are separated by 7.7" and 8.1 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 1104904736608017280 | 06:04:51.48 +66:41:26.6 (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 1104904736608017280,2461083.9934,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1104904736608017280 20260212.4934 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:50.55 +66:41:30.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.36 05:51:38.60 +65:02:26.9
148.38615 18.45286 galactic Cam Second-epoch detections are separated by 4.2" and 7.1 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 287903580680865408 | 05:51:39.61 +65:02:25.6 (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 287903580680865408,2461083.9934,12.36,0.05,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 287903580680865408 20260212.4934 12.36CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:38.60 +65:02:26.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.34 05:48:51.89 +65:44:00.4
147.59552 18.48558 galactic Cam Second-epoch detections are separated by 6.2" and 7.9 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 480244280760394496 | 05:48:53.45 +65:43:55.4 (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 480244280760394496,2461083.9934,12.34,0.05,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 480244280760394496 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:51.89 +65:44:00.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.41 05:51:04.25 +63:52:24.3
149.47014 17.89976 galactic Cam Second-epoch detections are separated by 8.6" and 8.1 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 286987550056405248 | 05:51:05.81 +63:52:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 286987550056405248,2461083.9934,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286987550056405248 20260212.4934 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:04.25 +63:52:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.53 05:56:18.99 +66:14:51.5
147.43291 19.38846 galactic Cam Second-epoch detections are separated by 3.4" and 6.8 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 480375706759819648 | 05:56:20.44 +66:14:44.5 (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 480375706759819648,2461083.9934,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480375706759819648 20260212.4934 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:18.99 +66:14:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.39 05:58:43.00 +56:41:18.7
156.66237 15.64144 galactic Cam Second-epoch detections are separated by 5.4" and 6.7 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 265621977543303552 | 05:58:43.60 +56:41:10.0 (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 265621977543303552,2461083.9934,12.39,0.05,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 265621977543303552 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:43.00 +56:41:18.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.60 05:53:14.24 +61:56:44.3
151.40696 17.29253 galactic Cam Second-epoch detections are separated by 6.5" and 7.6 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 283389436910588544 | 05:53:15.46 +61:56:42.2 (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 283389436910588544,2461083.9934,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 283389436910588544 20260212.4934 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:14.24 +61:56:44.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.61 05:40:59.59 +65:34:37.5
147.36605 17.68877 galactic Cam Second-epoch detections are separated by 0.6" and 7.0 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 480270772117070592 | 05:40:58.67 +65:34:39.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480270772117070592,2461083.9934,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 480270772117070592 20260212.4934 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:59.59 +65:34:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.64 05:45:37.71 +63:15:28.5
149.77027 17.08507 galactic Cam Second-epoch detections are separated by 3.4" and 6.2 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 286863859295386752 | 05:45:40.03 +63:15:29.9 (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 286863859295386752,2461083.9934,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286863859295386752 20260212.4934 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:37.71 +63:15:28.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.58 05:56:17.28 +66:10:13.0
147.50682 19.35483 galactic Cam Second-epoch detections are separated by 5.6" and 7.5 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 288220686706712064 | 05:56:18.78 +66:10:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 288220686706712064,2461083.9934,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 288220686706712064 20260212.4934 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:17.28 +66:10:13.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.67 05:51:18.08 +64:07:02.4
149.24987 18.02715 galactic Cam Second-epoch detections are separated by 6.3" and 5.9 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 287042186334934016 | 05:51:19.64 +64:06:59.1 (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 287042186334934016,2461083.9934,12.67,0.05,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 287042186334934016 20260212.4934 12.67CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:18.08 +64:07:02.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.75 05:44:44.44 +64:38:45.3
148.42479 17.62060 galactic Cam Second-epoch detections are separated by 2.6" and 7.2 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 287984570880687488 | 05:44:46.17 +64:38:47.9 (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 287984570880687488,2461083.9934,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287984570880687488 20260212.4934 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:44.44 +64:38:45.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 287777106780465280,2461083.9934,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287777106780465280 20260212.4934 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:27.83 +64:25:06.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 997535502008874240,2461083.9934,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 997535502008874240 20260212.4934 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:09.89 +57:00:13.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.86 05:52:03.90 +63:46:54.5
149.60649 17.95959 galactic Cam Second-epoch detections are separated by 5.0" and 6.1 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 286972298629071488 | 05:52:05.36 +63:46:54.8 (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 286972298629071488,2461083.9934,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286972298629071488 20260212.4934 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:03.90 +63:46:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.64 05:48:46.34 +65:49:37.5
147.50201 18.51710 galactic Cam Second-epoch detections are separated by 7.0" and 7.9 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 480248678806675840 | 05:48:48.54 +65:49:34.1 (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 480248678806675840,2461083.9934,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480248678806675840 20260212.4934 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:46.34 +65:49:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.77 05:49:33.21 +65:37:51.5
147.72516 18.50588 galactic Cam Second-epoch detections are separated by 1.9" and 6.6 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 | Large-amplitude variable Gaia DR2 288179184439631744 | 05:49:34.87 +65:37:52.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 288179184439631744,2461083.9934,12.77,0.05,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
Large-amplitude variable Gaia DR2 288179184439631744 20260212.4934 12.77CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:33.21 +65:37:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.80 05:50:26.45 +65:03:48.9
148.30772 18.34770 galactic Cam Second-epoch detections are separated by 6.7" and 7.9 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 288090673753754496 | 05:50:27.13 +65:03:43.9 (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 288090673753754496,2461083.9934,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 288090673753754496 20260212.4934 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:26.45 +65:03:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.63 05:47:07.84 +63:56:29.8
149.20743 17.53959 galactic Cam Second-epoch detections are separated by 8.4" and 8.1 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 | Large-amplitude variable Gaia DR2 286953744370711808 | 05:47:08.74 +63:56:25.8 (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)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 286953744370711808,2461083.9934,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 286953744370711808 20260212.4934 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:07.84 +63:56:29.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.84 05:50:24.85 +66:22:05.9
147.05898 18.89723 galactic Cam Second-epoch detections are separated by 7.5" and 6.4 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 480415495337678464 | 05:50:26.83 +66:22:02.0 (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 480415495337678464,2461083.9934,12.84,0.05,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 480415495337678464 20260212.4934 12.84CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:24.85 +66:22:05.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.93 05:48:38.89 +63:20:58.1
149.84247 17.42953 galactic Cam Second-epoch detections are separated by 8.8" and 8.1 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 286680034694440960 | 05:48:39.68 +63:20:36.8 (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 286680034694440960,2461083.9934,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286680034694440960 20260212.4934 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:38.89 +63:20:58.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
V0405 Cam,2461083.9934,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0405 Cam 20260212.4934 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:49.77 +64:25:14.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 480209096388326912,2461083.9934,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 480209096388326912 20260212.4934 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:38.32 +65:21:34.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.88 05:43:21.66 +64:09:25.3
148.81200 17.26738 galactic Cam Second-epoch detections are separated by 5.1" and 6.5 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 287749137953525760 | 05:43:22.00 +64:09:18.7 (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 287749137953525760,2461083.9934,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287749137953525760 20260212.4934 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:21.66 +64:09:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.91 05:45:42.88 +63:51:02.3
149.22021 17.35962 galactic Cam Second-epoch detections are separated by 7.2" and 7.7 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 286952335621597568 | 05:45:44.50 +63:51:01.6 (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 286952335621597568,2461083.9934,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286952335621597568 20260212.4934 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:42.88 +63:51:02.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.91 05:38:24.64 +65:46:08.7
147.05898 17.54064 galactic Cam Second-epoch detections are separated by 6.4" and 6.8 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 | ATO J084.5725+65.7660 | 05:38:23.35 +65:46:09.3 (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 J084.5725+65.7660,2461083.9934,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.5725+65.7660 20260212.4934 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:24.64 +65:46:08.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.95 05:39:37.56 +65:38:58.0
147.23080 17.59637 galactic Cam Second-epoch detections are separated by 4.0" and 7.6 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 480286818116221440 | 05:39:36.38 +65:39:00.6 (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 480286818116221440,2461083.9934,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480286818116221440 20260212.4934 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:37.56 +65:38:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 268735352093676928,2461083.9934,12.84,0.05,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 268735352093676928 20260212.4934 12.84CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:15.79 +57:36:17.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.87 05:58:19.46 +66:20:38.6
147.42394 19.61194 galactic Cam Second-epoch detections are separated by 8.5" and 7.8 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 480381719714898816 | 05:58:20.60 +66:20:34.6 (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 480381719714898816,2461083.9934,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 480381719714898816 20260212.4934 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:19.46 +66:20:38.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.96 05:50:17.37 +63:47:19.5
149.51138 17.78553 galactic Cam Second-epoch detections are separated by 5.1" and 5.9 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 286986145603664512 | 05:50:19.13 +63:47:19.8 (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 286986145603664512,2461083.9934,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286986145603664512 20260212.4934 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:17.37 +63:47:19.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.03 05:48:21.35 +65:41:24.6
147.61304 18.41973 galactic Cam Second-epoch detections are separated by 6.5" and 6.9 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 480243009450078080 | 05:48:23.35 +65:41:26.6 (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 480243009450078080,2461083.9934,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480243009450078080 20260212.4934 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:21.35 +65:41:24.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 1005438890372995456,2461083.9934,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1005438890372995456 20260212.4934 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:16.84 +59:12:35.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.98 05:55:23.87 +65:12:34.8
148.39720 18.88214 galactic Cam Second-epoch detections are separated by 4.7" and 6.7 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 287931931761713408 | 05:55:25.31 +65:12:29.7 (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 287931931761713408,2461083.9934,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287931931761713408 20260212.4934 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:23.87 +65:12:34.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.01 05:42:38.81 +63:52:35.2
149.03616 17.06996 galactic Cam Second-epoch detections are separated by 7.6" and 8.0 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 287694024933228928 | 05:42:40.62 +63:52:33.6 (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 287694024933228928,2461083.9934,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287694024933228928 20260212.4934 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:38.81 +63:52:35.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.11 05:39:28.70 +66:09:19.5
146.75154 17.81499 galactic Cam Second-epoch detections are separated by 7.6" and 8.0 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 480503181389030400 | 05:39:29.88 +66:09:29.0 (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 480503181389030400,2461083.9934,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480503181389030400 20260212.4934 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:28.70 +66:09:19.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.07 05:44:43.82 +65:26:08.8
147.68149 17.97131 galactic Cam Second-epoch detections are separated by 1.2" and 6.7 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 480232426650715648 | 05:44:45.76 +65:26:01.4 (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 480232426650715648,2461083.9934,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480232426650715648 20260212.4934 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:43.82 +65:26:08.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.21 05:59:51.56 +64:13:05.2
149.55932 18.91767 galactic Cam Second-epoch detections are separated by 4.0" and 6.6 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 287010914677359872 | 05:59:52.84 +64:13:12.3 (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 287010914677359872,2461083.9934,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287010914677359872 20260212.4934 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:51.56 +64:13:05.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.93 05:58:18.11 +57:06:15.9
156.24791 15.77178 galactic Cam Second-epoch detections are separated by 6.8" and 7.2 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 265704823168993024 | 05:58:17.73 +57:06:10.6 (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 265704823168993024,2461083.9934,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 265704823168993024 20260212.4934 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:18.11 +57:06:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 265619881599262720,2461083.9934,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 265619881599262720 20260212.4934 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:45.25 +56:42:01.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.01 05:54:20.42 +65:52:35.2
147.70646 19.05492 galactic Cam Second-epoch detections are separated by 3.5" and 6.9 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 288189320562343040 | 05:54:22.48 +65:52:28.2 (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 288189320562343040,2461083.9934,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 288189320562343040 20260212.4934 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:20.42 +65:52:35.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.23 05:52:41.14 +65:33:42.6
147.93519 18.77015 galactic Cam Second-epoch detections are separated by 5.7" and 7.6 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 288122417853843456 | 05:52:41.03 +65:33:30.1 (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 288122417853843456,2461083.9934,13.23,0.05,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 288122417853843456 20260212.4934 13.23CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:41.14 +65:33:42.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.19 05:41:03.60 +64:30:14.8
148.36956 17.20420 galactic Cam Second-epoch detections are separated by 3.2" and 6.8 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 287957048730287744 | 05:41:02.41 +64:29:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 287957048730287744,2461083.9934,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287957048730287744 20260212.4934 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:03.60 +64:30:14.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.25 05:39:56.82 +65:44:01.0
147.16822 17.66433 galactic Cam Second-epoch detections are separated by 4.7" and 7.4 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 480291010004296576 | 05:39:56.83 +65:43:50.1 (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 480291010004296576,2461083.9934,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480291010004296576 20260212.4934 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:56.82 +65:44:01.0 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.28 05:41:03.21 +64:30:02.1
148.37250 17.20195 galactic Cam Second-epoch detections are separated by 2.0" and 7.1 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 287957048730287744 | 05:41:02.41 +64:29:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 287957048730287744,2461083.9934,13.28,0.05,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 287957048730287744 20260212.4934 13.28CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:03.21 +64:30:02.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.20 05:45:18.02 +62:19:01.1
150.62921 16.62569 galactic Cam Second-epoch detections are separated by 7.3" and 7.7 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 286553281620131456 | 05:45:19.66 +62:19:09.1 (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 286553281620131456,2461083.9934,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286553281620131456 20260212.4934 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:18.02 +62:19:01.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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,2461083.9934,13.28,0.05,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
target 20260212.4934 13.28CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:49.38 +58:25:42.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.97 05:56:19.18 +56:48:39.3
156.39839 15.40010 galactic Cam Second-epoch detections are separated by 6.8" and 6.8 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 265682077022269440 | 05:56:18.06 +56:48:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 265682077022269440,2461083.9934,12.97,0.05,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 265682077022269440 20260212.4934 12.97CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:19.18 +56:48:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 286707591204897024,2461083.9934,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286707591204897024 20260212.4934 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:29.11 +63:08:01.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.37 05:45:50.72 +65:53:36.7
147.30236 18.27610 galactic Cam Second-epoch detections are separated by 4.8" and 6.9 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 480304990121058304 | 05:45:52.25 +65:53:36.3 (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 480304990121058304,2461083.9934,13.37,0.05,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 480304990121058304 20260212.4934 13.37CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:50.72 +65:53:36.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 286595406659053696,2461083.9934,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 286595406659053696 20260212.4934 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:35.64 +62:34:30.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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,2461083.9934,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:14.18 +65:11:50.3 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 480498199226971648,2461083.9934,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480498199226971648 20260212.4934 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:58.40 +66:02:22.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.54 05:39:17.37 +66:00:20.4
146.88210 17.72934 galactic Cam Second-epoch detections are separated by 2.1" and 6.5 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 480497855629601024 | 05:39:18.31 +66:00:22.8 (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 480497855629601024,2461083.9934,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480497855629601024 20260212.4934 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:17.37 +66:00:20.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.39 05:47:43.83 +65:46:26.0
147.50423 18.39784 galactic Cam Second-epoch detections are separated by 6.8" and 5.7 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 480248266489840256 | 05:47:44.12 +65:46:35.2 (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 480248266489840256,2461083.9934,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480248266489840256 20260212.4934 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:43.83 +65:46:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.70 05:48:10.40 +66:01:01.5
147.29334 18.54336 galactic Cam Second-epoch detections are separated by 4.8" and 6.2 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 480266099194017024 | 05:48:11.44 +66:00:57.4 (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 480266099194017024,2461083.9934,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480266099194017024 20260212.4934 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:10.40 +66:01:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.48 05:52:01.06 +64:51:10.8
148.58324 18.40952 galactic Cam Second-epoch detections are separated by 5.7" and 7.8 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 287885851055878656 | 05:52:02.76 +64:51:25.2 (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 287885851055878656,2461083.9934,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287885851055878656 20260212.4934 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:01.06 +64:51:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.74 06:08:04.30 +56:49:58.5
157.08907 16.86466 galactic Cam Second-epoch detections are separated by 4.3" and 7.6 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 | ATO J092.0171+56.8440 | 06:08:03.44 +56:49:52.0 (Gaia DR3) | CBF (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 J092.0171+56.8440,2461083.9934,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.0171+56.8440 20260212.4934 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:04.30 +56:49:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.54 05:55:54.78 +57:38:06.3
155.60570 15.71495 galactic Cam Second-epoch detections are separated by 6.6" and 6.8 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 268767890765975168 | 05:55:53.91 +57:38:00.8 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 268767890765975168,2461083.9934,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 268767890765975168 20260212.4934 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:54.78 +57:38:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 286865096245938432,2461083.9934,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 286865096245938432 20260212.4934 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:35.18 +63:18:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.64 05:44:53.17 +65:42:14.2
147.43609 18.10445 galactic Cam Second-epoch detections are separated by 7.9" and 8.2 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 480254279444102784 | 05:44:54.63 +65:42:11.4 (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 480254279444102784,2461083.9934,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480254279444102784 20260212.4934 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:53.17 +65:42:14.2 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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,2461083.9934,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.66 +64:03:09.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 265658982981523840,2461083.9934,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 265658982981523840 20260212.4934 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:17.18 +56:45:18.1 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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,2461083.9934,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:21.21 +65:21:31.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.82 06:02:54.00 +56:56:46.9
156.67576 16.26908 galactic Cam Second-epoch detections are separated by 3.7" and 6.4 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 997525400245826688 | 06:02:53.32 +56:56:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 997525400245826688,2461083.9934,13.82,0.05,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 997525400245826688 20260212.4934 13.82CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:54.00 +56:56:46.9 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 13.79 06:04:35.78 +57:23:54.7
156.34802 16.66724 galactic Cam Second-epoch detections are separated by 2.7" and 7.3 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 | 06:04:35.78 +57:23:54.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461083.9934,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.4934 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:35.78 +57:23:54.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.98 07:14:41.40 +63:49:31.7
152.34643 26.67866 galactic Cam Second-epoch detections are separated by 0.5" and 6.5 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 J108.6772+63.8214 | 07:14:41.40 +63:49:31.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.6772+63.8214,2461083.9934,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.6772+63.8214 20260212.4934 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:41.40 +63:49:31.7 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 J0659453+573010,2461083.9934,11.13,0.05,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
NSVS J0659453+573010 20260212.4934 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:45.36 +57:30:10.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 J0708263+633826,2461083.9934,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0708263+633826 20260212.4934 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:08:26.21 +63:38:26.6 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 J0608359+640759,2461083.9934,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0608359+640759 20260212.4934 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:36.36 +64:07:57.5 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.4934 2461083.9934 12.51 05:48:53.89 +66:06:43.4
147.23595 18.65044 galactic Cam Second-epoch detections are separated by 3.3" and 7.2 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 480407760099088768 | 05:48:55.69 +66:06:42.5 (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 480407760099088768,2461083.9934,12.51,0.05,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 480407760099088768 20260212.4934 12.51CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.89 +66:06:43.4 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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 J0637343+621930,2461083.9934,12.01,0.05,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
NSVS J0637343+621930 20260212.4934 12.01CV 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:34.42 +62:19:25.8 ;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-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20_00sec_-14_90C_LIGHT_0490_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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
DK Lyn,2461083.9934,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DK Lyn 20260212.4934 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:48.85 +57:15:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20_00sec_-15_00C_LIGHT_0047_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: 2461032.89256047 23.12.2025 09:25:07.225 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
First image: 2461032.89256047 23.12.2025 09:25:07.225 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Last image: 2461083.99370542 12.02.2026 11:50:46.148 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 6 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): 15666
Objects passed selection criteria: 15616
Measurements per detected object (mean, median, min, max): 3.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 2.5 2 4
Average stars detected per image: 11976.5
Average stars matched: 11721.8 (97.8729 %)
Memory usage VmPeak: 120924 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 06:12:36 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: 2461032.89256047 23.12.2025 09:25:07.225 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
First image: 2461032.89256047 23.12.2025 09:25:07.225 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Last image: 2461083.99370542 12.02.2026 11:50:46.148 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 510
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 56 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): 90883
Objects passed selection criteria: 90673
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 70230.8
Average stars matched: 67261.2 (95.7718 %)
Memory usage VmPeak: 1866156 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 06:15:58 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.china-vo.org
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.china-vo.org)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Cam-10-Q2b1x1
#######################################
########### Starting Cam-10-Q2b1x1 ###########
Processing Cam-10-Q2b1x1
server tau has sufficient free disk space available: 1158182 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1158182 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.png' -> 'transient_report/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits_preview.png'
Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
renamed 'Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.png' -> 'transient_report/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits_preview.png'
Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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= 550.8024
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 663.6139
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1618.3931
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 622.7551
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1619.8016
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 620.7540
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.93825
INFO: SECOND_EPOCH__SD_ratio= 0.003
----------------------------------------------
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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
SExtractor catalog cache: saved Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat to cache
SExtractor catalog cache: saved Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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: 2461083.99311642
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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits exists and is non-empty
Saving wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits to local_wcs_cache/
'wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits' -> 'local_wcs_cache/wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits'
wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
Saving wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits to local_wcs_cache/
'wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits' -> 'local_wcs_cache/wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits'
wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits'
wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:28.546 +61:59:48.89
Second-epoch image center 06:51:29.684 +62:00:09.56
Angular distance between the image centers 0.01 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 06:51:28.546 +61:59:48.89
Second-epoch image center 06:51:28.594 +62:00:48.24
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 06:51:29.684 +62:00:09.56
Second-epoch second image center 06:51:28.594 +62:00:48.24
Angular distance between the image centers 0.01095 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits &> /tmp/tmp.FQBGhWZMef
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.jrVGWGFlky
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.ktP4jzMruF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.kLPssQTsFv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
Found non-empty wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
The reference image (wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits) and catalog (wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat) found
'wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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 8390 out of 16399 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.963249
a=0.000000 b=1.000000 c=22.963249
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
2.2 pix Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
2.5 pix Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
2.6 pix Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Limiting magnitude estimates:
15.4 mag. Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
15.4 mag. Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
14.3 mag. Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
14.2 mag. Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
All-image limiting magnitude estimate: 14.2 (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.FQBGhWZMef (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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits' -> 'wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1168, passed=16399
Got 16399 stars (including 15214 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
util/solve_plate_with_UCAC5 got 16399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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: 0.30"
Estimated accuracy of the plate solution: 0.28"
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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits -region wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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.jrVGWGFlky (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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits' -> 'wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1171, passed=16357
Got 16357 stars (including 15161 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 16357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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: 0.30"
Estimated accuracy of the plate solution: 0.28"
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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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.ktP4jzMruF (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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=690, passed=7733
Got 7733 stars (including 7042 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 7733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 961 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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.kLPssQTsFv (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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=658, passed=7682
Got 7682 stars (including 7022 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 7682 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 962 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out11057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20950.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 53s
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: 11s
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Considering the candidate 20795_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20795_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:05.51 +65:55:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.175 288201896226549888 089.02477053690 +65.91840817279 10.7326 10.2718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20796_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20796_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:25.43 +62:41:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.828 283679123864254208 087.85432468067 +62.69819330826 10.1601 9.7637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20798_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20798_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:30.78 +60:07:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.298 282249483870939008 087.88060427501 +60.12444648571 9.8850 9.4771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20799_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20799_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:01.92 +64:24:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 2.833 287086922716138880 088.75961815805 +64.41066600202 10.2574 9.9345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20800_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20800_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20801_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20801_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20802_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20802_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:36.52 +59:35:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 2.705 270120083909050112 089.65073164144 +59.58816916990 9.7334 9.2929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20803_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20803_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20804_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20804_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:01.46 +63:09:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 4.615 286699069989905920 088.50327971825 +63.15949267876 9.8662 9.4561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20805_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20805_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:54.27 +64:53:24.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)
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Considering the candidate 20807_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20807_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20809_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20809_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:06.70 +59:47:45.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20810_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20810_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:51.88 +62:14:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 2.996 283418230371223040 089.21438042086 +62.24694368907 9.4424 9.0728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20811_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20811_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:22.60 +60:51:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)
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Considering the candidate 20812_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20812_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20813_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20813_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:05.45 +58:31:52.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20814_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20814_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:49:58.08 +60:34:12.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20815_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20815_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:03.49 +59:01:45.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20816_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20816_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 20817_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20817_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:27.32 +65:41:49.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20832_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20832_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:45:53.47 +63:17:44.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20844_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20844_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:02.64 +65:56:46.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20846_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20846_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:52.94 +63:03:20.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20849_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20849_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:49.09 +64:44:34.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20855_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20855_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:43.54 +65:09:38.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20857_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20857_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:02.10 +65:36:49.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20864_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20864_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:41.37 +65:49:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.35, MAG_FAINT_SEARCH_LIMIT=11.33)GAIADR2_OUTPUT=# 4.428 480262422702056832 086.67536529788 +65.82330262052 9.1601 8.8574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20866_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20866_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20867_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20867_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:50.72 +65:04:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 2.182 288036454083668096 085.96276923446 +65.07990689161 9.3338 9.1850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20868_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20868_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:45:46.91 +60:53:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 0.740 1087644018957050624 116.44532149252 +60.89533340372 10.5513 9.7797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20877_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20877_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:10.18 +66:11:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 3.822 480494174840350208 085.79493580223 +66.18377981536 9.4174 9.1655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20881_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20881_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20886_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20886_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20889_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20889_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 20890_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20890_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:28.88 +65:55:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 1.047 480299462499916160 085.37091756415 +65.92530558960 9.5847 9.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20891_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20891_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:37:48.27 +65:55:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.898 480121169817761024 084.45309739829 +65.92415845692 9.3376 8.9680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20899_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20899_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:01.75 +64:55:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 3.744 288039649541160960 085.25970450625 +64.92033847477 9.6486 9.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20902_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20902_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:59:45.38 +57:30:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 0.777 1000590078453940608 104.93910804466 +57.50272891475 11.8970 10.6531 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20910_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20910_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20916_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20916_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:44.19 +65:06:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 5.521 288012604130323456 086.93748194208 +65.11143101661 10.1059 9.7878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20917_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20917_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20918_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20918_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20949_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20949_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:15.83 +66:04:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 0.100 480489506213119104 085.81589553195 +66.07295578718 10.2759 9.8630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20950_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 20950_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 20959_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20959_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 20983_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 20983_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:58:09.46 +63:13:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.272 1100185082944333824 104.53924916893 +63.23147423392 12.2327 11.7762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11496_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 11496_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 11057_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 11057_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 13085_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 13085_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 65s
Prepared the HTML report for the field Cam-10-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 ####
06:40:46.74 +59:52:04.1
06:04:02.69 +59:32:22.3
06:58:04.96 +58:29:17.2
05:56:34.37 +59:18:10.5
05:53:18.26 +61:26:49.6
05:52:29.33 +63:09:38.1
05:58:18.38 +57:54:01.6
05:52:42.43 +60:44:34.8
05:42:49.25 +64:06:54.4
05:48:25.58 +63:43:14.4
05:49:45.58 +65:56:14.3
05:49:30.30 +63:19:37.7
05:55:56.65 +64:29:48.6
05:56:48.35 +66:15:45.9
05:46:30.08 +64:46:41.0
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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
SExtractor catalog cache: saved Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat to cache
SExtractor catalog cache: saved Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Creating symlink local_wcs_cache/wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Creating symlink local_wcs_cache/wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
Creating symlink local_wcs_cache/wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits exists and is non-empty
wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:28.546 +61:59:48.89
Second-epoch image center 06:51:29.684 +62:00:09.56
Angular distance between the image centers 0.01 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 06:51:28.546 +61:59:48.89
Second-epoch image center 06:51:28.594 +62:00:48.24
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 06:51:29.684 +62:00:09.56
Second-epoch second image center 06:51:28.594 +62:00:48.24
Angular distance between the image centers 0.01095 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits &> /tmp/tmp.a11PIyeyWJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.dAVZv1VB9g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.TiSVUsaQN3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.eO2HVQxPzZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
Found non-empty wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits and wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
The reference image (wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits) and catalog (wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat) found
'wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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 8463 out of 97352 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.856163
a=0.000000 b=1.000000 c=22.856163
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 455 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
2.0 pix Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
2.5 pix Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
2.5 pix Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Limiting magnitude estimates:
15.6 mag. Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
15.6 mag. Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
14.5 mag. Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
14.5 mag. Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.9 (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.a11PIyeyWJ (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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits' -> 'wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=7021, passed=97336
Got 97336 stars (including 90181 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat
util/solve_plate_with_UCAC5 got 97336 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 967 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-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits -region wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-25-07_20.00sec_-14.90C_LIGHT_0490.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.dAVZv1VB9g (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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits' -> 'wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6988, passed=97578
Got 97578 stars (including 90417 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 97578 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2025-12-23_03-26-09_20.00sec_-14.90C_LIGHT_0491.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.TiSVUsaQN3 (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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=3717, passed=44202
Got 44202 stars (including 40442 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 44202 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 960 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-49-55_20.00sec_-15.00C_LIGHT_0047.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.eO2HVQxPzZ (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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=3678, passed=44103
Got 44103 stars (including 40380 good ones) from the SExtractor catalog wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 44103 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 964 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-10-Q2b1x1_055956_TTUQ2b1x1_5513_wUYPbI6c/Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out115028.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out116245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64821.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 396s
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: 89s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115028_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115028_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:39:30.42 +65:08:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.135 1089559780531259008 114.87669665785 +65.13996982079 14.3334 13.7122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115030_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115030_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:14.41 +57:36:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.701 268952879301024640 088.30797783091 +57.60552726484 11.7929 11.0433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115033_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115033_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:41.53 +58:20:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.887 269037266817555840 088.92615655240 +58.33669889584 12.0872 11.5486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115037_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115037_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:06.57 +65:11:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.029 287876750021991552 089.77471622636 +65.19492438230 12.7687 12.2082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115042_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115042_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:27.90 +56:56:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.297 997476433322372736 091.11674929382 +56.94831921330 12.1843 11.7004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115043_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115043_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:05:10.27 +65:44:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.292 1008771239535605504 091.29199811754 +65.73853910590 13.0687 12.5929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115047_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115047_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:01:15.29 +65:24:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.224 1008655309778206848 090.31373112720 +65.41195101924 12.7722 12.0803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115053_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115053_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:04.79 +62:11:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.201 283557833989039744 086.76844263468 +62.18709977780 12.1557 11.7061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115056_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115056_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:03:18.93 +59:16:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.405 999634023030245760 090.83143631143 +59.26740329316 12.4142 12.0253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115057_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115057_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:03:16.51 +65:44:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.408 1008750928632847488 090.81963390435 +65.73973445322 12.4812 11.7640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115058_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115058_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:01:49.44 +66:15:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.708 1102428876939425664 105.45641312475 +66.26653400654 14.1760 13.7528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115059_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115059_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:17.64 +62:05:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.639 283511585781410944 087.07231954643 +62.08541930688 12.0363 11.5130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115061_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115061_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:18.92 +58:26:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.739 269812010198283136 088.08023205317 +58.44134635433 11.6899 11.1983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115063_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115063_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:31.68 +61:08:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.547 282513985137581568 089.13158924618 +61.13820206376 12.1217 11.5799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115064_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115064_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:51.15 +62:32:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.467 283662425031425920 087.71401180751 +62.54044940888 12.2811 11.7292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115065_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115065_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:15.18 +57:28:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.204 268754108213634560 088.81351244370 +57.48098473769 11.8628 11.3574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115066_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115066_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115067_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115067_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:12:05.79 +56:59:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.588 998790315358568192 093.02180340895 +56.98568320541 12.0667 11.6066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115069_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115069_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 115071_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115071_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:57.43 +61:36:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.856 283293160924154112 086.73868910286 +61.61067852485 11.9277 11.4220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115073_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115073_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:42.74 +65:34:25.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 115078_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115078_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:59.50 +66:29:23.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 115079_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115079_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 115080_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115080_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:18.08 +65:05:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.415 287909627994816512 088.07548797324 +65.09325126840 12.0197 11.5458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115084_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115084_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:03:18.90 +57:38:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.864 999064402992011008 090.83073992642 +57.63574787949 12.0487 11.5085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115085_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115085_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:02.95 +59:49:20.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 115086_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115086_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:37.12 +59:10:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.850 269905777925407104 089.15566866240 +59.17997817421 11.5727 11.0963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115087_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115087_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115088_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115088_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:01:18.32 +57:53:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.500 999087943707747840 090.32741147516 +57.88491347164 12.0494 11.5107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115089_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115089_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 115090_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115090_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:23.60 +64:19:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.027 287024113114370304 089.35025955609 +64.31787749253 12.7678 12.2541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115091_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115091_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:39:44.49 +56:35:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.672 986229082205756928 114.93503915202 +56.58866937128 13.5682 12.9080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115092_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115092_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:15.33 +61:13:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.762 283222070625684736 086.81604568924 +61.22556906055 11.9335 11.4657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115093_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115093_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:40.11 +64:15:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.111 287013938334334336 089.66646077079 +64.25122382844 12.4553 11.8749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115096_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115096_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:15.17 +59:05:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.460 270080325396186240 088.06424694746 +59.09809043157 11.7552 11.2660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115098_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115098_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:54.05 +65:12:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.779 287911968753734016 088.47384629238 +65.20703605962 12.1720 11.4546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115099_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115099_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:03:50.77 +66:25:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.033 1104873297447466368 090.96038483381 +66.41604601027 12.4988 11.9596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115100_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115100_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:06.36 +61:36:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.161 283282371963653120 087.52735776750 +61.61430932688 11.8630 11.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115101_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115101_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:00:22.02 +57:26:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.858 999048906748735872 090.09351937359 +57.44096405503 11.6709 11.3835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115103_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115103_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:02:12.98 +59:36:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.772 999736827367985024 090.55627545353 +59.60144800597 12.1609 11.7517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115104_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115104_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:11.08 +58:16:15.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 115105_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115105_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115106_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115106_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:29.98 +61:57:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.647 283395656023249408 088.12518580899 +61.95397704270 12.1423 11.6196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115107_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115107_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:45.38 +57:35:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 5.576 268776373324089472 089.44155941439 +57.58606266581 11.4701 10.9016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115109_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115109_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:00:57.20 +56:45:43.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 115113_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115113_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:06:17.07 +60:16:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.116 1005739748539299200 091.57312342997 +60.27651278199 12.5142 12.0068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115115_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115115_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:28.73 +66:14:06.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 115116_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115116_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 115117_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115117_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:13.53 +64:18:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.522 287061530869528320 088.30622292976 +64.31175979575 12.0639 11.3492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115119_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115119_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:08.45 +66:13:30.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 115120_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115120_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:06:07.58 +56:47:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.228 997459184734579584 091.53066802247 +56.79241833284 11.8392 11.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115121_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115121_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:11.29 +64:00:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.439 286819432153053056 089.54794166657 +64.00536941292 12.3007 11.8191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115122_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115122_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:45.86 +62:58:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.345 283701801291651840 089.43915771282 +62.97506251681 12.2956 11.9128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115126_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115126_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:39.26 +57:59:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.694 269022977463609472 088.41321992518 +57.99900962843 11.5119 11.0468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115127_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115127_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115128_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115128_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:19.39 +57:09:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.214 268698827691990656 088.58242958815 +57.15859047047 11.3772 10.9285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115129_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115129_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:10.43 +60:48:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.926 282298682718560896 089.54569129167 +60.81346888843 12.0422 11.4875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:30.05 +64:00:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.384 287037612194085504 087.87743836096 +64.01060658899 12.0377 11.6886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115131_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115131_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:23.01 +57:52:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.848 999121135215514880 091.09822496445 +57.88067719027 11.7732 11.3247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115132_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115132_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115133_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115133_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:47.48 +60:22:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.778 282260169749685888 088.70048860033 +60.37939295444 11.8303 11.3983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115134_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115134_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115135_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115135_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115136_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115136_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:06.32 +64:54:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.746 287889394405846912 088.27714799943 +64.91443724038 12.1478 11.7361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115138_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115138_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:23.08 +59:51:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.793 270174883395152768 088.84825974453 +59.85701787735 11.7806 11.4341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115140_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115140_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:16.48 +62:40:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.796 286624062678546176 086.06959199892 +62.67895633995 11.4994 11.1692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115141_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115141_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115142_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115142_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:02.25 +58:47:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.889 269826960980938112 088.76042832993 +58.78551540826 11.6273 11.1254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115143_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115143_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:03.37 +58:25:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.677 269073722499956224 089.01376546328 +58.42331280053 11.7902 11.4028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115144_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115144_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:07.38 +65:27:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.669 288106990331321728 088.52963467842 +65.46160040925 11.9896 11.5803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115145_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115145_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:08:40.90 +58:30:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 115146_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115146_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:54.64 +63:28:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.885 286739167804675456 089.22734394398 +63.48119920686 12.1859 11.6849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115147_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115147_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115148_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115148_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:55.37 +64:12:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.714 287054757703519616 087.98089022333 +64.20709578008 12.0213 11.5452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115149_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115149_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:29.91 +66:36:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.430 480445628827186304 089.12458520475 +66.61093634461 12.2163 11.6941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115150_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115150_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:00.65 +59:01:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.743 270076893717967616 088.00498306939 +59.03346576850 11.1955 10.9263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115152_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115152_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115153_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115153_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115154_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115154_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:24.08 +61:53:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.801 283388303039225472 088.35101524533 +61.89524446956 11.8262 11.3124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115156_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115156_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:00:38.05 +57:02:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.546 997535089692007936 090.15825378020 +57.04067749525 11.2853 10.8079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115157_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115157_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:17.37 +57:27:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.521 268773658904768000 089.07251080488 +57.45620829355 11.4153 10.8908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115158_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115158_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:49:52.47 +60:45:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.204 282436297768201600 087.46920862933 +60.76581380553 11.6422 11.0974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115159_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115159_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:11:48.23 +57:52:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.149 999307811673626112 092.95206455939 +57.87732471694 12.0052 11.5996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115160_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115160_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:45:27.63 +62:14:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.439 283549622011589888 086.36371404956 +62.24619510386 11.7754 11.2478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115162_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115162_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115163_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115163_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:17.99 +59:57:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.461 282183027839542272 088.32686314524 +59.95628734418 11.6930 11.1326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115166_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115166_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:59.50 +61:38:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.531 283329960203540224 087.99774891041 +61.64373689592 11.7319 11.1668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115168_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115168_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115169_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115169_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:03.86 +57:08:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.024 265706055823058304 089.76762918053 +57.14669970390 11.3364 10.8763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115170_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115170_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:02:30.70 +66:17:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.857 1104877351896633600 090.62973763308 +66.29016591425 12.3138 11.7697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115172_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115172_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:09:11.52 +56:49:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.181 998773552101714560 092.29818101883 +56.81995874951 11.7432 11.3821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115173_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115173_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:52.42 +58:57:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.867 269855612706230144 089.46995302313 +58.95517082578 11.7115 11.2904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115174_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115174_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:46.40 +61:18:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.238 282567929926571264 089.19347716571 +61.30846538506 11.9404 11.4170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115175_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115175_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:16.43 +59:07:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.384 269861282064224000 089.57082554482 +59.12780731285 11.7544 11.2688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115176_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115176_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:29.93 +65:08:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.620 287917225793835648 089.12437191014 +65.13534803433 12.0108 11.4986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115177_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115177_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115178_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115178_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:49.13 +65:19:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.239 1008642287437310848 091.20524859159 +65.32092658576 12.2763 11.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115179_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115179_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:09:33.92 +65:35:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.148 1008705092741834240 092.38922124793 +65.58367347713 12.4059 11.8763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115183_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115183_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115185_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115185_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:05:50.95 +65:52:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.428 1008732752331242496 091.46257194648 +65.87094058095 12.2214 11.6786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115186_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115186_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 115188_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115188_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:00:09.46 +58:25:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.329 999198685144707584 090.03852834989 +58.42308963840 11.5409 11.0796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115190_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115190_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:42.39 +61:45:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.439 283334804926578560 088.67629767735 +61.75993720901 12.0330 11.5509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115191_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115191_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:53.69 +65:11:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.689 288096544972174592 087.72354351620 +65.18548388149 11.8362 11.2903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115192_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115192_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:43.78 +65:42:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.300 288195230437355008 088.68342768523 +65.71482183213 11.8531 11.3701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115193_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115193_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:19.99 +57:00:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 115194_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115194_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115197_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115197_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:08.13 +61:22:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.151 282568788917170048 089.28260542065 +61.37315713158 11.8203 11.3518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115198_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115198_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:21.90 +60:28:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.494 282261097462428032 088.84259958554 +60.46797369715 11.7973 11.3261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115200_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115200_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 115201_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115201_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:59.59 +61:52:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.051 283491038657881984 087.24756199848 +61.88232362604 11.5100 11.0228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115202_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115202_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115203_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115203_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:49.74 +63:08:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.870 286753255297198080 087.70711814556 +63.14792859296 11.7160 11.2225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115205_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115205_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:38.56 +60:07:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.148 270204677584716160 089.16008127721 +60.11894078528 11.6759 11.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115206_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115206_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:56.29 +65:22:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.348 288116374838023168 087.98471438619 +65.36867570436 11.8964 11.4062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115207_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115207_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:49:59.01 +61:59:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.122 283493478199265280 087.49475820198 +61.98775366327 11.5108 11.0828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115208_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115208_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:55:38.57 +58:53:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.347 269828850766528768 088.91144621369 +58.89594329865 11.4369 11.0766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115209_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115209_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115210_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115210_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:36.26 +64:45:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.993 287881629105024512 087.90231615213 +64.76257585265 11.7290 11.2578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115211_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115211_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115212_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115212_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115213_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115213_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:22.63 +63:20:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.515 286760608281172224 087.84345220473 +63.34893795406 11.6199 11.1636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115214_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115214_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:04.05 +66:08:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.322 480494350936237184 085.51770271251 +66.14719854581 11.3048 10.8349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115215_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115215_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 115216_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115216_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:15.50 +60:12:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.036 270211820113931904 089.56402587955 +60.20989390796 11.6370 11.2799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115217_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115217_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:02.71 +63:43:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.230 286795071098604032 089.26122944140 +63.71727570573 11.8915 11.4840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115218_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115218_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115219_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115219_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:37.33 +61:08:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.732 283212552975627264 087.15281931524 +61.14209606380 11.6218 11.0189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115220_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115220_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:19.90 +63:03:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.027 286702746481939968 088.08353886074 +63.05317887645 11.4471 10.6970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115221_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115221_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:38.66 +63:03:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.355 286703193158632192 087.91025369326 +63.05020395376 11.6066 11.1061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115222_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115222_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:40.01 +64:43:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.963 287100387437507968 089.41776861250 +64.72030395354 11.8622 11.3859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115223_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115223_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:32.21 +59:21:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.362 270145986856196608 087.88676831609 +59.35860722013 11.2852 10.7825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115224_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115224_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:05.73 +63:05:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.897 286668592901634560 086.77161794533 +63.09774012458 11.4485 10.8895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115225_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115225_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:59.92 +62:48:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.513 283637411139813504 089.99905927912 +62.80326770937 11.8333 11.4814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115226_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115226_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:24.11 +63:20:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.976 286902823238730752 085.85129048066 +63.33795793964 11.3978 10.9618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115228_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115228_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:16.09 +64:12:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.022 287013044981139584 089.56959197077 +64.20729736610 11.7769 11.2230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115229_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115229_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:02:39.35 +59:03:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.408 999628692975300736 090.66465304276 +59.06579843913 11.5713 11.1799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115230_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115230_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:01:49.08 +61:46:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.989 1005985897407058432 090.45556615058 +61.77042008727 12.0114 11.5577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115231_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115231_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:26.14 +57:44:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 115232_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115232_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:13.06 +63:13:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.926 286860968779703936 086.80137950118 +63.23298960645 11.3611 10.8678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115233_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115233_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:57.15 +59:26:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 115234_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115234_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:44.71 +62:55:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.153 286653990012866944 086.68602650657 +62.93042540995 11.4263 10.9643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115235_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115235_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:52.64 +59:01:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.320 269854581915251200 089.21865045201 +59.01743774228 11.3046 11.0013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115236_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115236_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:59:44.70 +62:34:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.299 283440839079395328 089.93528971674 +62.57990041614 11.6676 11.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115238_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115238_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:23.77 +57:47:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.001 999118730033839488 091.10014616047 +57.78909027986 11.4588 10.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115239_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115239_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:29.81 +58:13:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.371 269008546373413760 089.12254816355 +58.22008153652 10.9602 10.6401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115240_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115240_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:40.96 +61:59:11.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 115242_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115242_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:47.65 +63:51:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.550 286987588712661760 087.69951798972 +63.86460609522 11.4202 10.8148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115243_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115243_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:07.14 +62:09:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.335 283372085242575872 089.52836594054 +62.15536479010 11.7909 11.3438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115245_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115245_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:34.96 +66:02:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 3.418 288215605762135296 089.14487942894 +66.04738363691 11.5453 11.0536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115246_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115246_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:07:09.17 +57:54:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.567 999135050909463040 091.79006316588 +57.90193747754 11.4872 11.0665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115247_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115247_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:49.15 +61:10:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.594 1005885914866132352 091.20308027095 +61.16771603399 11.8252 11.3435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115250_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115250_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:22.41 +63:13:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.112 286675464849255552 087.09458168173 +63.21699380205 11.3562 10.7832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115251_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115251_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:42.19 +59:35:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.804 270164545410449280 087.92293977003 +59.59633723261 10.7120 10.4920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115253_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115253_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:18.57 +59:34:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.968 270117919245538944 089.32546182886 +59.57814062478 11.0743 10.8715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115254_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115254_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:06:32.06 +57:18:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.877 998997749394755328 091.63254598433 +57.30737762030 11.2474 10.8401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115256_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115256_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115257_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115257_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:48.50 +61:55:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.444 283386550692537984 088.70273369314 +61.92241157844 11.4251 10.9566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115259_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115259_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115260_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115260_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:05.46 +60:27:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.580 282264018039937280 088.52363386762 +60.46344766272 11.1192 10.6131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115261_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115261_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:15.05 +61:35:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 5.761 282587240099484672 089.31605398707 +61.59527658715 11.5082 10.9629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115262_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115262_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:29.72 +66:24:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.204 480392646110644480 089.12479025951 +66.41313086517 11.5073 11.0324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115264_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115264_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115267_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115267_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115268_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115268_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115270_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115270_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:36.37 +65:57:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.277 288205229118389760 089.39864707510 +65.96347892385 11.1542 10.6750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115273_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115273_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:27.86 +65:02:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.778 287870496549629696 089.61987120536 +65.04695397282 11.5432 11.1172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115274_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115274_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115275_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115275_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115276_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115276_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 115278_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115278_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:37.16 +59:25:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 5.746 270103896176692352 088.65253247383 +59.42152596664 10.3642 10.2161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115279_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115279_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115280_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115280_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:25.34 +64:43:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.551 1008597035662101120 091.10789146142 +64.72145826252 11.6081 11.1632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115281_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115281_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:18.12 +61:13:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.944 282551883928857728 088.07389723540 +61.21970138652 11.0206 10.7291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115282_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115282_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:50:25.77 +57:32:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.738 1000742326454461568 102.60761478687 +57.54664602698 12.2959 11.5023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115284_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115284_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:02.66 +63:01:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.520 286693572431775616 088.50961035747 +63.02854057083 11.1424 10.9740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115285_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115285_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115288_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115288_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 115289_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115289_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:15.28 +59:55:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 3.662 282197360147851264 087.81193790818 +59.92918904813 10.4606 10.1619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115290_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115290_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 115291_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115291_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115292_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115292_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115295_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115295_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:02:31.87 +66:09:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 5.368 1008798280649460096 090.63500612101 +66.15825170554 11.1033 10.6518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115298_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115298_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115299_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115299_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115300_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115300_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 115301_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115301_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 115302_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115302_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 115303_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115303_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:03:42.35 +57:38:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 4.420 999069389449111680 090.92525984812 +57.63784209526 10.1501 9.9227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115304_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115304_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:06:19.28 +66:36:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.235 1104856392456115584 091.57960532988 +66.60349018851 11.0491 10.6755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115305_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115305_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:23.24 +66:41:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.282 1104899067251197056 091.09623859391 +66.68407263868 10.8946 10.4354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115306_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115306_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:25.38 +59:49:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.036 282102114952935936 087.60488542799 +59.82855463132 10.1361 9.7177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115307_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115307_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:28.51 +58:16:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.878 269010367439518848 089.36728602646 +58.27421387113 10.1366 9.7911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115308_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115308_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115309_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115309_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115310_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115310_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:02.39 +60:11:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.580 282206809075857280 088.50751387545 +60.18440223436 10.0671 9.7907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115313_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115313_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:38:47.44 +65:01:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.632 1103585597532337920 099.69843515153 +65.03256668429 11.8537 10.9706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115314_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115314_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:34.16 +59:18:07.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115315_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115315_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:18.34 +61:26:47.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115317_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115317_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:18.43 +57:54:01.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115318_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115318_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:06.88 +59:47:45.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115319_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115319_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 115320_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115320_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 115322_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115322_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:49:55.85 +60:34:06.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115323_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115323_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115324_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115324_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:27.19 +65:41:49.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115326_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115326_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:01.27 +65:45:14.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115337_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115337_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:45:53.54 +63:17:43.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115351_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115351_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:52.91 +63:03:18.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115356_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115356_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:51.98 +65:07:51.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115360_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115360_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:02.72 +65:56:46.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115362_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115362_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:48.87 +64:44:34.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115365_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115365_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:43.67 +65:09:38.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115371_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115371_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:02.08 +65:36:51.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 115375_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115375_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:09.24 +65:21:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 5.408 288116134319853312 088.04179579626 +65.35675415877 9.2819 9.0905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115381_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115381_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115386_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115386_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:48.86 +64:06:53.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115393_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115393_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:50.67 +65:04:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 2.498 288036454083668096 085.96276923446 +65.07990689161 9.3338 9.1850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115397_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115397_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:25.28 +63:43:18.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115399_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115399_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115410_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115410_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115414_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115414_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:10.17 +66:11:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 3.909 480494174840350208 085.79493580223 +66.18377981536 9.4174 9.1655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115438_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115438_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:37:48.24 +65:55:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 3.081 480121169817761024 084.45309739829 +65.92415845692 9.3376 8.9680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115444_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115444_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:28.83 +65:55:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.309 480299462499916160 085.37091756415 +65.92530558960 9.5847 9.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115449_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115449_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115461_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115461_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115462_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115462_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115464_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115464_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:00.13 +63:09:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 4.673 286699069989905920 088.50327971825 +63.15949267876 9.8662 9.4561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115470_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115470_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115480_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115480_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:47.93 +66:15:48.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115485_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115485_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115492_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115492_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:28.17 +65:00:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 5.750 287867953929027968 089.12115528780 +65.01127488803 10.3269 9.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115495_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115495_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115501_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115501_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:48.23 +62:52:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 2.981 286608188481574784 087.20243150639 +62.87646014943 10.1084 9.7903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115524_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115524_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115529_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115529_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115530_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115530_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115547_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115547_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115549_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115549_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:13.42 +64:56:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.579 288040508534633472 085.05554168846 +64.94811284534 9.9793 9.2718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115551_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115551_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115553_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115553_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115561_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115561_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:16.63 +62:13:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 4.428 283569344501400192 086.57146764254 +62.22900202700 10.1275 9.6959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115563_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115563_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:15.42 +66:04:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.403 480489506213119104 085.81589553195 +66.07295578718 10.2759 9.8630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115572_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115572_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115573_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115573_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115576_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115576_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:29.50 +64:46:41.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115591_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115591_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 115595_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115595_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115603_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115603_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115613_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115613_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:22.85 +64:44:53.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)
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Considering the candidate 115619_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115619_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115626_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115626_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:46:36.34 +57:11:02.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115630_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115630_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115633_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115633_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115638_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115638_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115639_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115639_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115642_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115642_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115647_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115647_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 115655_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115655_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115657_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115657_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115663_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115663_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115667_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115667_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115668_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115668_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115674_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115674_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115678_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115678_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115692_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115692_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:17.35 +66:08:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 5.664 480490876305467392 085.82618196313 +66.14397282044 10.6179 10.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115695_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115695_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115706_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115706_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115708_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115708_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115709_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115709_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115725_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115725_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:00.08 +66:07:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.467 480499573616500096 084.99822680019 +66.11769742245 10.5863 9.8041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115729_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115729_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115731_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115731_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:02:22.19 +57:04:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.712 997527186952218752 090.59277084275 +57.06810105267 10.4759 10.1105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115733_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115733_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 115736_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115736_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115742_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115742_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115753_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115753_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 115754_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115754_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115775_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115775_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:22:21.71 +59:52:33.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115777_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115777_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115783_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115783_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115794_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115794_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115801_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115801_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115823_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115823_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115825_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115825_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:28.18 +65:25:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.836 480222221806818048 085.11793129780 +65.43146305343 11.0003 10.6768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115850_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115850_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115853_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115853_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115857_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115857_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:22:27.58 +59:54:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 115861_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115861_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:27.79 +66:02:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 5.046 480321590171401600 086.11850070513 +66.04424231331 11.0463 10.5211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115870_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115870_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:15.72 +56:38:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.045 265630331256305536 089.06485896542 +56.64595328005 10.6640 9.9054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115872_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115872_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115875_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115875_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:01:52.24 +56:50:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.465 997506330591062016 090.46641945820 +56.83285311542 10.8202 10.1508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115876_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115876_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115899_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115899_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:39.88 +66:10:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.307 480362753138388352 087.66841930930 +66.17209758682 11.5177 11.0784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115909_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115909_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115918_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115918_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115922_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115922_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115927_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115927_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115929_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115929_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 115946_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115946_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115947_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115947_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:37.03 +65:54:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.073 480308052434629504 086.15447526143 +65.91617751017 11.2643 10.5150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115949_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115949_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115952_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115952_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:09:31.80 +60:44:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.531 1098897451749333248 107.38225364163 +60.74119629303 13.4752 12.9984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115955_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115955_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115956_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115956_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 115957_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115957_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115959_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115959_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 115964_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115964_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 115967_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115967_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:56.44 +64:18:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.740 287774491143172352 086.23779946222 +64.30413688714 11.2163 10.7937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115979_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115979_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:18.38 +65:24:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.140 288106474935247616 088.32717768939 +65.40848513252 11.5984 11.1183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 115983_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 115983_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 115996_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 115996_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116001_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116001_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:12.36 +65:31:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 5.242 480228062963795968 085.54855715814 +65.51921252671 11.1765 10.6200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116005_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116005_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:41.98 +66:20:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.069 480417591280786944 087.92684662642 +66.34144898399 11.4649 11.0549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116009_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116009_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116011_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116011_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116020_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116020_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116025_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116025_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116032_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116032_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:04.04 +64:51:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.971 287994363406100224 086.77008068884 +64.86603514034 11.4498 10.9245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116034_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116034_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:10:05.22 +65:56:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.085 1101665025595447808 107.52450947067 +65.94017376089 11.4804 9.6934 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116043_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116043_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:38:45.36 +65:41:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.640 480289188938174080 084.69010056279 +65.68342669731 11.3078 11.0577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116048_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116048_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116051_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116051_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116062_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116062_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116064_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116064_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116069_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116069_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:45.72 +65:25:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.871 480232426650715648 086.19067358098 +65.43371215218 11.3946 10.9820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116075_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116075_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:57:42.37 +57:14:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.422 268706936590364288 089.42654415017 +57.23814496398 11.0067 10.7103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116077_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116077_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:38.12 +64:56:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.161 288031124029854336 085.90873152170 +64.94362273714 11.3782 10.6195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116080_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116080_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116081_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116081_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 116087_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116087_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116089_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116089_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:38:26.60 +66:15:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.956 1095822564406401792 114.61085449231 +66.25687649142 13.2475 12.7117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116093_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116093_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116094_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116094_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:32:37.13 +57:49:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.482 1004339005084796672 098.15364072975 +57.83099861079 12.6434 12.0572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116098_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116098_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:58:02.77 +60:46:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.015 1003011688391034752 104.51044945427 +60.77113217072 13.6945 13.3216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116103_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116103_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116116_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116116_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:17:20.86 +58:01:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.572 990305800739981184 109.33721578425 +58.02920762817 13.2215 12.7308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116117_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116117_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116118_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116118_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 116120_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116120_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:22:39.63 +66:02:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.404 1101810229849763456 110.66622416973 +66.04664196645 13.5954 13.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116123_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116123_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116125_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116125_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:53.49 +63:27:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.443 286775550471277952 087.72608184264 +63.46185013457 11.6269 11.1649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116127_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116127_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:39:10.07 +65:25:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.851 480268332577220096 084.78981863806 +65.42767695650 11.4197 10.5712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116132_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116132_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:12.90 +65:02:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.068 288044906581129216 085.05508712367 +65.04180194106 11.3510 10.8837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116135_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116135_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:12:26.30 +62:14:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.280 1099088148297470848 108.10957188604 +62.24075549112 13.4747 12.9794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116141_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116141_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116149_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116149_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116155_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116155_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:39.66 +65:37:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.314 480230296346935168 085.91612871233 +65.62868140369 11.6726 10.8759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116158_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116158_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116163_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116163_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116165_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116165_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116167_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116167_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:46:37.35 +57:44:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.054 1001507586550761856 101.65467416409 +57.74568922699 13.0397 12.3420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116178_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116178_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116184_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116184_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116198_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116198_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 116203_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116203_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:20.18 +63:30:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.326 286915055305361152 085.58734183127 +63.50049616374 11.4943 11.0390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116210_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116210_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116212_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116212_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116213_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116213_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 116219_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116219_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:13:27.24 +61:01:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.568 1086912809365606144 108.36415775104 +61.03344377789 14.2389 13.7021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116225_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116225_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116235_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116235_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:45.48 +63:56:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.210 286980132649504768 088.69258400178 +63.94253714438 11.8039 11.3437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116245_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116245_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:51.07 +65:11:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.745 288049751304149248 085.96103020651 +65.18985431440 11.7620 11.0625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116248_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116248_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 116249_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116249_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116253_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116253_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:17.25 +65:16:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.321 480216311933330688 085.07147684192 +65.27858955097 11.5996 11.1968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116265_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116265_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116273_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116273_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116278_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116278_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:39:51.54 +65:41:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.632 480287677109676672 084.96390603383 +65.68889338474 11.6135 11.0915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116285_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116285_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:37.88 +65:40:15.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 116288_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116288_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:01.23 +64:46:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.288 287981890820946944 085.75580823564 +64.76979239950 11.7160 11.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116293_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116293_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:53:11.88 +62:57:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.503 1100119765081627904 103.29827807053 +62.96090699346 13.9220 13.2900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116301_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116301_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116316_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116316_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:39.66 +66:08:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.903 480314988804916224 087.16857808890 +66.14526471339 12.1116 11.7498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116317_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116317_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116320_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116320_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:52:32.63 +65:47:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.763 288187289039906304 088.13686458021 +65.78312571404 11.8512 11.2919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116330_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116330_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:49:22.07 +66:04:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.337 480360554115161472 087.34408312946 +66.08054661510 11.9297 11.4551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116332_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116332_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116335_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116335_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:09.81 +63:42:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.375 286971714513544576 087.79360644477 +63.71498561679 12.0257 11.6247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116338_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116338_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116340_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116340_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:40:16.37 +65:20:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.957 480217617603382272 085.06881001560 +65.33769865246 11.5908 11.2434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116343_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116343_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:52:34.41 +62:46:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.065 1100087707445753728 103.14484484417 +62.76726410614 13.9288 13.4679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116366_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116366_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116373_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116373_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116382_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116382_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116393_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116393_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:45:31.85 +65:09:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.410 288061090017789184 086.38488405565 +65.15427606235 11.9483 11.4738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116401_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116401_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:44:22.25 +66:07:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.616 480325885138694912 086.09248704229 +66.12819909742 11.7778 11.2695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116409_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116409_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:22.46 +63:43:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.964 286982602254072704 087.59633753196 +63.72041203992 12.0400 11.7307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116413_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116413_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:54:17.15 +64:03:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.105 286994323221290880 088.57405950677 +64.05059644190 11.8726 11.3579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116414_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116414_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:50:39.59 +66:23:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.988 480427349444775936 087.66675058655 +66.39194441737 12.0675 11.5286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116416_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116416_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:46:19.43 +66:22:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.682 480526301196567424 086.58267554440 +66.37815896213 11.9756 11.4938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116437_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116437_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:45:49.99 +64:43:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.657 1088741228483208320 116.45871794552 +64.72765421608 13.6962 13.2152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116445_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116445_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 116447_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116447_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:39:46.09 +65:03:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.327 480197345357817984 084.94032493335 +65.05917548631 11.6268 10.8472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116459_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116459_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116507_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116507_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:15.49 +65:12:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.081 480200399078103040 085.31382805733 +65.20188417683 11.6469 11.1312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116509_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116509_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 116524_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116524_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:39:44.25 +65:31:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.362 480273344802651264 084.93385523502 +65.53297793793 11.8885 11.2495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116527_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116527_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 116534_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116534_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:17.86 +66:05:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.710 480316092613346048 086.82552852278 +66.09442792669 12.0202 11.5037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116542_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116542_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116550_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116550_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:08:51.33 +66:03:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.540 1101678322814125312 107.21464868939 +66.06062381539 13.9296 13.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116552_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116552_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:40.94 +65:00:21.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 116555_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116555_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:50:47.95 +57:11:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.622 1000356161650928640 102.69966799214 +57.19689620678 13.5907 13.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116559_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116559_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116561_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116561_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:38:53.15 +65:48:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.044 480479507529333248 084.72020435575 +65.81668626602 11.8986 11.3326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116570_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116570_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:26.86 +65:05:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.179 288047724079625472 085.61157415987 +65.09806700132 11.6635 11.2788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116572_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116572_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116577_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116577_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:56.57 +65:47:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.326 480293823206510976 085.48243133654 +65.78613194922 11.9141 11.4936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116582_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116582_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116583_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116583_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:58:21.01 +56:54:09.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 116591_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116591_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:43:56.92 +66:03:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.339 480324369013277312 085.98719612173 +66.05556620942 12.0324 11.4156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116605_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116605_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:47:43.15 +66:18:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.427 480335226690812288 086.93276993652 +66.31438290642 12.1204 11.7070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116607_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116607_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116617_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116617_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:38:19.24 +65:58:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.874 480496687398512128 084.58143377251 +65.97934657269 11.6487 11.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116628_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116628_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116632_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116632_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116686_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116686_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116692_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116692_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:51:52.73 +65:50:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.819 288191893244843904 087.97302310831 +65.84525971958 12.2355 11.7304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116699_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116699_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:41:03.36 +57:04:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116706_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116706_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116711_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116711_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116713_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116713_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:38:48.04 +66:08:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.054 480548742402117504 084.69860118107 +66.14014777178 11.6378 10.8613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116730_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116730_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:48:11.38 +66:18:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.979 480335402786191104 087.04849348999 +66.31336686217 12.1841 11.6252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116738_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116738_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116747_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116747_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116750_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116750_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:14.28 +65:14:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.575 480203697612985216 085.30959999985 +65.24510358263 12.2439 11.4575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116761_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116761_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:42:55.03 +63:38:20.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 116793_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116793_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 116820_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116820_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:41:54.53 +64:26:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.538 287958796779680000 085.47825403380 +64.44218048755 12.2656 11.7010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116830_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116830_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116851_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116851_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 116864_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116864_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:53:44.33 +57:35:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.146 268952260825734400 088.43257378818 +57.58417079456 11.7934 11.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116866_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116866_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116903_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116903_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116967_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 116967_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 116968_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116968_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 116999_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 116999_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 117031_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 117031_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 05:56:44.01 +56:55:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.401 265695541743132928 089.18148380650 +56.91678946124 11.8570 11.1807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117038_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 117038_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 117051_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 117051_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 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 117121_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 117121_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 117197_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 117197_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 26729_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 26729_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 91171_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 91171_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:40:46.74 +59:52:04.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 64821_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 64821_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 29559_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 29559_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 88529_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 88529_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:04:02.65 +59:32:22.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 27404_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 27404_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 07748_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 07748_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 44790_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 44790_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 65218_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 65218_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 07:46:13.47 +57:28:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.813 1082412542633189760 116.55652344504 +57.47942856247 12.7645 12.2622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107530_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 107530_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048
The candidate 81130_Cam-10-Q2b1x1_2026-02-12_05-50-46_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
**** FOUND 06:58:04.94 +58:29:17.4 in the exclusion list exclusion_list_local.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 18s
make_report_in_HTML.sh TOTAL: 503s
Prepared the HTML report for the field Cam-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:40:46.74 +59:52:04.1
06:04:02.69 +59:32:22.3
06:58:04.96 +58:29:17.2
05:56:34.37 +59:18:10.5
05:53:18.26 +61:26:49.6
05:52:29.33 +63:09:38.1
05:58:18.38 +57:54:01.6
05:52:42.43 +60:44:34.8
05:42:49.25 +64:06:54.4
05:48:25.58 +63:43:14.4
05:49:45.58 +65:56:14.3
05:49:30.30 +63:19:37.7
05:55:56.65 +64:29:48.6
05:56:48.35 +66:15:45.9
05:46:30.08 +64:46:41.0
05:48:53.89 +66:06:43.4
06:19:48.85 +57:15:19.1
05:57:09.07 +57:09:59.9
05:49:59.24 +64:14:24.6
05:53:06.27 +59:24:32.4
05:51:47.53 +59:52:00.9
05:52:17.47 +60:03:51.8
06:05:32.40 +57:59:30.5
06:02:27.28 +57:35:01.1
05:53:30.54 +65:20:10.2
05:56:36.66 +59:10:44.8
06:06:55.09 +66:06:35.7
06:10:57.32 +60:41:12.7
05:58:55.34 +60:24:53.8
05:59:46.47 +61:04:53.4
06:14:47.33 +64:03:15.6
05:52:04.84 +58:38:05.8
06:10:06.93 +57:10:09.0
05:49:20.22 +62:43:51.2
05:50:15.91 +61:27:35.6
05:50:16.33 +63:20:32.3
05:56:13.16 +64:32:17.8
05:49:06.93 +60:10:40.6
05:58:34.70 +59:04:15.6
05:52:38.74 +58:36:48.2
05:48:08.13 +60:41:41.2
06:03:52.87 +57:16:15.7
05:56:41.98 +59:24:23.7
05:46:40.91 +65:49:25.3
05:47:09.37 +65:06:35.0
05:41:01.02 +64:55:13.4
05:52:26.91 +63:09:39.7
05:47:43.75 +65:06:43.1
05:48:53.22 +63:58:13.1
05:58:16.10 +65:30:13.1
05:54:14.98 +65:04:06.9
05:55:23.95 +58:00:33.0
05:56:29.09 +66:29:22.0
05:52:53.12 +65:20:49.6
05:55:47.91 +64:54:56.9
05:52:10.92 +64:17:55.7
05:54:35.49 +66:18:21.9
05:56:04.10 +65:55:08.6
05:54:49.11 +66:31:53.0
05:57:26.87 +57:25:23.9
05:48:53.92 +65:58:49.5
05:53:19.26 +66:17:40.9
05:53:48.84 +66:15:04.4
05:50:05.51 +66:07:57.6
05:53:57.43 +64:35:48.4
05:50:32.44 +64:16:13.9
05:46:04.73 +65:59:45.4
05:57:16.53 +63:54:56.9
05:54:49.56 +63:46:24.3
05:45:56.54 +65:07:38.0
05:54:39.86 +61:58:47.2
05:56:01.74 +57:22:49.0
05:52:44.53 +63:42:44.0
06:04:50.55 +66:41:30.9
05:51:38.60 +65:02:26.9
05:48:51.89 +65:44:00.4
05:51:04.25 +63:52:24.3
05:56:18.99 +66:14:51.5
05:58:43.00 +56:41:18.7
05:53:14.24 +61:56:44.3
05:40:59.59 +65:34:37.5
05:45:37.71 +63:15:28.5
05:56:17.28 +66:10:13.0
05:51:18.08 +64:07:02.4
05:44:44.44 +64:38:45.3
05:46:27.83 +64:25:06.2
06:00:09.89 +57:00:13.6
05:52:03.90 +63:46:54.5
05:48:46.34 +65:49:37.5
05:49:33.21 +65:37:51.5
05:50:26.45 +65:03:48.9
05:47:07.84 +63:56:29.8
05:50:24.85 +66:22:05.9
05:48:38.89 +63:20:58.1
05:42:49.77 +64:25:14.5
05:43:38.32 +65:21:34.3
05:43:21.66 +64:09:25.3
05:45:42.88 +63:51:02.3
05:38:24.64 +65:46:08.7
05:39:37.56 +65:38:58.0
05:58:15.79 +57:36:17.7
05:58:19.46 +66:20:38.6
05:50:17.37 +63:47:19.5
05:48:21.35 +65:41:24.6
06:16:16.84 +59:12:35.5
05:55:23.87 +65:12:34.8
05:42:38.81 +63:52:35.2
05:39:28.70 +66:09:19.5
05:44:43.82 +65:26:08.8
05:59:51.56 +64:13:05.2
05:58:18.11 +57:06:15.9
05:59:45.25 +56:42:01.6
05:54:20.42 +65:52:35.2
05:52:41.14 +65:33:42.6
05:41:03.60 +64:30:14.8
05:39:56.82 +65:44:01.0
05:41:03.21 +64:30:02.1
05:45:18.02 +62:19:01.1
06:25:49.38 +58:25:42.5
05:56:19.18 +56:48:39.3
05:51:29.11 +63:08:01.1
05:45:50.72 +65:53:36.7
05:45:35.64 +62:34:30.8
05:50:14.18 +65:11:50.3
05:39:58.40 +66:02:22.7
05:39:17.37 +66:00:20.4
05:47:43.83 +65:46:26.0
05:48:10.40 +66:01:01.5
05:52:01.06 +64:51:10.8
06:08:04.30 +56:49:58.5
05:55:54.78 +57:38:06.3
05:46:35.18 +63:18:35.9
05:44:53.17 +65:42:14.2
05:48:53.66 +64:03:09.8
05:55:17.18 +56:45:18.1
05:51:21.21 +65:21:31.9
06:02:54.00 +56:56:46.9
06:04:35.78 +57:23:54.7
07:14:41.40 +63:49:31.7
06:08:36.36 +64:07:57.5
07:08:26.21 +63:38:26.6
06:37:34.42 +62:19:25.8
06:59:45.36 +57:30:10.5
########### Completed Cam-10-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 ####
05:56:34.37 +59:18:10.5
05:53:18.26 +61:26:49.6
05:52:29.33 +63:09:38.1
05:58:18.38 +57:54:01.6
05:52:42.43 +60:44:34.8
05:42:49.25 +64:06:54.4
05:48:25.58 +63:43:14.4
05:49:45.58 +65:56:14.3
05:49:30.30 +63:19:37.7
05:55:56.65 +64:29:48.6
05:56:48.35 +66:15:45.9
05:46:30.08 +64:46:41.0
06:04:02.69 +59:32:22.3
06:40:46.74 +59:52:04.1
06:58:04.96 +58:29:17.2
05:57:09.07 +57:09:59.9
05:49:59.24 +64:14:24.6
05:53:06.27 +59:24:32.4
05:51:47.53 +59:52:00.9
05:52:17.47 +60:03:51.8
06:05:32.40 +57:59:30.5
06:02:27.28 +57:35:01.1
05:53:30.54 +65:20:10.2
05:56:36.66 +59:10:44.8
06:06:55.09 +66:06:35.7
06:10:57.32 +60:41:12.7
05:58:55.34 +60:24:53.8
05:59:46.47 +61:04:53.4
06:14:47.33 +64:03:15.6
05:52:04.84 +58:38:05.8
06:10:06.93 +57:10:09.0
05:49:20.22 +62:43:51.2
05:50:15.91 +61:27:35.6
05:50:16.33 +63:20:32.3
05:56:13.16 +64:32:17.8
05:49:06.93 +60:10:40.6
05:58:34.70 +59:04:15.6
05:52:38.74 +58:36:48.2
05:48:08.13 +60:41:41.2
06:03:52.87 +57:16:15.7
05:56:41.98 +59:24:23.7
05:46:40.91 +65:49:25.3
05:47:09.37 +65:06:35.0
05:41:01.02 +64:55:13.4
05:52:26.91 +63:09:39.7
05:47:43.75 +65:06:43.1
05:48:53.22 +63:58:13.1
05:58:16.10 +65:30:13.1
05:54:14.98 +65:04:06.9
05:55:23.95 +58:00:33.0
05:56:29.09 +66:29:22.0
05:52:53.12 +65:20:49.6
05:55:47.91 +64:54:56.9
05:52:10.92 +64:17:55.7
05:54:35.49 +66:18:21.9
05:56:04.10 +65:55:08.6
05:54:49.11 +66:31:53.0
05:57:26.87 +57:25:23.9
05:48:53.92 +65:58:49.5
05:53:19.26 +66:17:40.9
05:53:48.84 +66:15:04.4
05:50:05.51 +66:07:57.6
05:53:57.43 +64:35:48.4
05:50:32.44 +64:16:13.9
05:46:04.73 +65:59:45.4
05:57:16.53 +63:54:56.9
05:54:49.56 +63:46:24.3
05:45:56.54 +65:07:38.0
05:54:39.86 +61:58:47.2
05:56:01.74 +57:22:49.0
05:52:44.53 +63:42:44.0
06:04:50.55 +66:41:30.9
05:51:38.60 +65:02:26.9
05:48:51.89 +65:44:00.4
05:51:04.25 +63:52:24.3
05:56:18.99 +66:14:51.5
05:58:43.00 +56:41:18.7
05:53:14.24 +61:56:44.3
05:40:59.59 +65:34:37.5
05:45:37.71 +63:15:28.5
05:56:17.28 +66:10:13.0
05:51:18.08 +64:07:02.4
05:44:44.44 +64:38:45.3
05:46:27.83 +64:25:06.2
06:00:09.89 +57:00:13.6
05:52:03.90 +63:46:54.5
05:48:46.34 +65:49:37.5
05:49:33.21 +65:37:51.5
05:50:26.45 +65:03:48.9
05:47:07.84 +63:56:29.8
05:50:24.85 +66:22:05.9
05:48:38.89 +63:20:58.1
05:42:49.77 +64:25:14.5
05:43:38.32 +65:21:34.3
05:43:21.66 +64:09:25.3
05:45:42.88 +63:51:02.3
05:38:24.64 +65:46:08.7
05:39:37.56 +65:38:58.0
05:58:15.79 +57:36:17.7
05:58:19.46 +66:20:38.6
05:50:17.37 +63:47:19.5
05:48:21.35 +65:41:24.6
06:16:16.84 +59:12:35.5
05:55:23.87 +65:12:34.8
05:42:38.81 +63:52:35.2
05:39:28.70 +66:09:19.5
05:44:43.82 +65:26:08.8
05:59:51.56 +64:13:05.2
05:58:18.11 +57:06:15.9
05:59:45.25 +56:42:01.6
05:54:20.42 +65:52:35.2
05:52:41.14 +65:33:42.6
05:41:03.60 +64:30:14.8
05:39:56.82 +65:44:01.0
05:41:03.21 +64:30:02.1
05:45:18.02 +62:19:01.1
06:25:49.38 +58:25:42.5
05:56:19.18 +56:48:39.3
05:51:29.11 +63:08:01.1
05:45:50.72 +65:53:36.7
05:45:35.64 +62:34:30.8
05:50:14.18 +65:11:50.3
05:39:58.40 +66:02:22.7
05:39:17.37 +66:00:20.4
05:47:43.83 +65:46:26.0
05:48:10.40 +66:01:01.5
05:52:01.06 +64:51:10.8
06:08:04.30 +56:49:58.5
05:55:54.78 +57:38:06.3
05:46:35.18 +63:18:35.9
05:44:53.17 +65:42:14.2
05:48:53.66 +64:03:09.8
05:55:17.18 +56:45:18.1
05:51:21.21 +65:21:31.9
06:02:54.00 +56:56:46.9
06:04:35.78 +57:23:54.7
07:14:41.40 +63:49:31.7
06:59:45.36 +57:30:10.5
07:08:26.21 +63:38:26.6
06:08:36.36 +64:07:57.5
05:48:53.89 +66:06:43.4
06:37:34.42 +62:19:25.8
06:19:48.85 +57:15:19.1
###################################################################################
05:56:34.37 +59:18:10.5 -- not an asteroid (will add it to exclusion list)
05:53:18.26 +61:26:49.6 -- not an asteroid (will add it to exclusion list)
05:52:29.33 +63:09:38.1 -- not an asteroid (will add it to exclusion list)
05:58:18.38 +57:54:01.6 -- not an asteroid (will add it to exclusion list)
05:52:42.43 +60:44:34.8 -- not an asteroid (will add it to exclusion list)
05:42:49.25 +64:06:54.4 -- not an asteroid (will add it to exclusion list)
05:48:25.58 +63:43:14.4 -- not an asteroid (will add it to exclusion list)
05:49:45.58 +65:56:14.3 -- not an asteroid (will add it to exclusion list)
05:49:30.30 +63:19:37.7 -- not an asteroid (will add it to exclusion list)
05:55:56.65 +64:29:48.6 -- not an asteroid (will add it to exclusion list)
05:56:48.35 +66:15:45.9 -- not an asteroid (will add it to exclusion list)
05:46:30.08 +64:46:41.0 -- not an asteroid (will add it to exclusion list)
06:04:02.69 +59:32:22.3 -- not an asteroid (will add it to exclusion list)
06:40:46.74 +59:52:04.1 -- not an asteroid (will add it to exclusion list)
06:58:04.96 +58:29:17.2 -- not an asteroid (will add it to exclusion list)
05:57:09.07 +57:09:59.9 -- not an asteroid (will add it to exclusion list)
05:49:59.24 +64:14:24.6 -- not an asteroid (will add it to exclusion list)
05:53:06.27 +59:24:32.4 -- not an asteroid (will add it to exclusion list)
05:51:47.53 +59:52:00.9 -- not an asteroid (will add it to exclusion list)
05:52:17.47 +60:03:51.8 -- not an asteroid (will add it to exclusion list)
06:05:32.40 +57:59:30.5 -- not an asteroid (will add it to exclusion list)
06:02:27.28 +57:35:01.1 -- not an asteroid (will add it to exclusion list)
05:53:30.54 +65:20:10.2 -- not an asteroid (will add it to exclusion list)
05:56:36.66 +59:10:44.8 -- not an asteroid (will add it to exclusion list)
06:06:55.09 +66:06:35.7 -- not an asteroid (will add it to exclusion list)
06:10:57.32 +60:41:12.7 -- not an asteroid (will add it to exclusion list)
05:58:55.34 +60:24:53.8 -- not an asteroid (will add it to exclusion list)
05:59:46.47 +61:04:53.4 -- not an asteroid (will add it to exclusion list)
06:14:47.33 +64:03:15.6 -- not an asteroid (will add it to exclusion list)
05:52:04.84 +58:38:05.8 -- not an asteroid (will add it to exclusion list)
06:10:06.93 +57:10:09.0 -- not an asteroid (will add it to exclusion list)
05:49:20.22 +62:43:51.2 -- not an asteroid (will add it to exclusion list)
05:50:15.91 +61:27:35.6 -- not an asteroid (will add it to exclusion list)
05:50:16.33 +63:20:32.3 -- not an asteroid (will add it to exclusion list)
05:56:13.16 +64:32:17.8 -- not an asteroid (will add it to exclusion list)
05:49:06.93 +60:10:40.6 -- not an asteroid (will add it to exclusion list)
05:58:34.70 +59:04:15.6 -- not an asteroid (will add it to exclusion list)
05:52:38.74 +58:36:48.2 -- not an asteroid (will add it to exclusion list)
05:48:08.13 +60:41:41.2 -- not an asteroid (will add it to exclusion list)
06:03:52.87 +57:16:15.7 -- not an asteroid (will add it to exclusion list)
05:56:41.98 +59:24:23.7 -- not an asteroid (will add it to exclusion list)
05:46:40.91 +65:49:25.3 -- not an asteroid (will add it to exclusion list)
05:47:09.37 +65:06:35.0 -- not an asteroid (will add it to exclusion list)
05:41:01.02 +64:55:13.4 -- not an asteroid (will add it to exclusion list)
05:52:26.91 +63:09:39.7 -- not an asteroid (will add it to exclusion list)
05:47:43.75 +65:06:43.1 -- not an asteroid (will add it to exclusion list)
05:48:53.22 +63:58:13.1 -- not an asteroid (will add it to exclusion list)
05:58:16.10 +65:30:13.1 -- not an asteroid (will add it to exclusion list)
05:54:14.98 +65:04:06.9 -- not an asteroid (will add it to exclusion list)
05:55:23.95 +58:00:33.0 -- not an asteroid (will add it to exclusion list)
05:56:29.09 +66:29:22.0 -- not an asteroid (will add it to exclusion list)
05:52:53.12 +65:20:49.6 -- not an asteroid (will add it to exclusion list)
05:55:47.91 +64:54:56.9 -- not an asteroid (will add it to exclusion list)
05:52:10.92 +64:17:55.7 -- not an asteroid (will add it to exclusion list)
05:54:35.49 +66:18:21.9 -- not an asteroid (will add it to exclusion list)
05:56:04.10 +65:55:08.6 -- not an asteroid (will add it to exclusion list)
05:54:49.11 +66:31:53.0 -- not an asteroid (will add it to exclusion list)
05:57:26.87 +57:25:23.9 -- not an asteroid (will add it to exclusion list)
05:48:53.92 +65:58:49.5 -- not an asteroid (will add it to exclusion list)
05:53:19.26 +66:17:40.9 -- not an asteroid (will add it to exclusion list)
05:53:48.84 +66:15:04.4 -- not an asteroid (will add it to exclusion list)
05:50:05.51 +66:07:57.6 -- not an asteroid (will add it to exclusion list)
05:53:57.43 +64:35:48.4 -- not an asteroid (will add it to exclusion list)
05:50:32.44 +64:16:13.9 -- not an asteroid (will add it to exclusion list)
05:46:04.73 +65:59:45.4 -- not an asteroid (will add it to exclusion list)
05:57:16.53 +63:54:56.9 -- not an asteroid (will add it to exclusion list)
05:54:49.56 +63:46:24.3 -- not an asteroid (will add it to exclusion list)
05:45:56.54 +65:07:38.0 -- not an asteroid (will add it to exclusion list)
05:54:39.86 +61:58:47.2 -- not an asteroid (will add it to exclusion list)
05:56:01.74 +57:22:49.0 -- not an asteroid (will add it to exclusion list)
05:52:44.53 +63:42:44.0 -- not an asteroid (will add it to exclusion list)
06:04:50.55 +66:41:30.9 -- not an asteroid (will add it to exclusion list)
05:51:38.60 +65:02:26.9 -- not an asteroid (will add it to exclusion list)
05:48:51.89 +65:44:00.4 -- not an asteroid (will add it to exclusion list)
05:51:04.25 +63:52:24.3 -- not an asteroid (will add it to exclusion list)
05:56:18.99 +66:14:51.5 -- not an asteroid (will add it to exclusion list)
05:58:43.00 +56:41:18.7 -- not an asteroid (will add it to exclusion list)
05:53:14.24 +61:56:44.3 -- not an asteroid (will add it to exclusion list)
05:40:59.59 +65:34:37.5 -- not an asteroid (will add it to exclusion list)
05:45:37.71 +63:15:28.5 -- not an asteroid (will add it to exclusion list)
05:56:17.28 +66:10:13.0 -- not an asteroid (will add it to exclusion list)
05:51:18.08 +64:07:02.4 -- not an asteroid (will add it to exclusion list)
05:44:44.44 +64:38:45.3 -- not an asteroid (will add it to exclusion list)
05:46:27.83 +64:25:06.2 -- not an asteroid (will add it to exclusion list)
06:00:09.89 +57:00:13.6 -- not an asteroid (will add it to exclusion list)
05:52:03.90 +63:46:54.5 -- not an asteroid (will add it to exclusion list)
05:48:46.34 +65:49:37.5 -- not an asteroid (will add it to exclusion list)
05:49:33.21 +65:37:51.5 -- not an asteroid (will add it to exclusion list)
05:50:26.45 +65:03:48.9 -- not an asteroid (will add it to exclusion list)
05:47:07.84 +63:56:29.8 -- not an asteroid (will add it to exclusion list)
05:50:24.85 +66:22:05.9 -- not an asteroid (will add it to exclusion list)
05:48:38.89 +63:20:58.1 -- not an asteroid (will add it to exclusion list)
05:42:49.77 +64:25:14.5 -- not an asteroid (will add it to exclusion list)
05:43:38.32 +65:21:34.3 -- not an asteroid (will add it to exclusion list)
05:43:21.66 +64:09:25.3 -- not an asteroid (will add it to exclusion list)
05:45:42.88 +63:51:02.3 -- not an asteroid (will add it to exclusion list)
05:38:24.64 +65:46:08.7 -- not an asteroid (will add it to exclusion list)
05:39:37.56 +65:38:58.0 -- not an asteroid (will add it to exclusion list)
05:58:15.79 +57:36:17.7 -- not an asteroid (will add it to exclusion list)
05:58:19.46 +66:20:38.6 -- not an asteroid (will add it to exclusion list)
05:50:17.37 +63:47:19.5 -- not an asteroid (will add it to exclusion list)
05:48:21.35 +65:41:24.6 -- not an asteroid (will add it to exclusion list)
06:16:16.84 +59:12:35.5 -- not an asteroid (will add it to exclusion list)
05:55:23.87 +65:12:34.8 -- not an asteroid (will add it to exclusion list)
05:42:38.81 +63:52:35.2 -- not an asteroid (will add it to exclusion list)
05:39:28.70 +66:09:19.5 -- not an asteroid (will add it to exclusion list)
05:44:43.82 +65:26:08.8 -- not an asteroid (will add it to exclusion list)
05:59:51.56 +64:13:05.2 -- not an asteroid (will add it to exclusion list)
05:58:18.11 +57:06:15.9 -- not an asteroid (will add it to exclusion list)
05:59:45.25 +56:42:01.6 -- not an asteroid (will add it to exclusion list)
05:54:20.42 +65:52:35.2 -- not an asteroid (will add it to exclusion list)
05:52:41.14 +65:33:42.6 -- not an asteroid (will add it to exclusion list)
05:41:03.60 +64:30:14.8 -- not an asteroid (will add it to exclusion list)
05:39:56.82 +65:44:01.0 -- not an asteroid (will add it to exclusion list)
05:41:03.21 +64:30:02.1 -- not an asteroid (will add it to exclusion list)
05:45:18.02 +62:19:01.1 -- not an asteroid (will add it to exclusion list)
06:25:49.38 +58:25:42.5 -- not an asteroid (will add it to exclusion list)
05:56:19.18 +56:48:39.3 -- not an asteroid (will add it to exclusion list)
05:51:29.11 +63:08:01.1 -- not an asteroid (will add it to exclusion list)
05:45:50.72 +65:53:36.7 -- not an asteroid (will add it to exclusion list)
05:45:35.64 +62:34:30.8 -- not an asteroid (will add it to exclusion list)
05:50:14.18 +65:11:50.3 -- not an asteroid (will add it to exclusion list)
05:39:58.40 +66:02:22.7 -- not an asteroid (will add it to exclusion list)
05:39:17.37 +66:00:20.4 -- not an asteroid (will add it to exclusion list)
05:47:43.83 +65:46:26.0 -- not an asteroid (will add it to exclusion list)
05:48:10.40 +66:01:01.5 -- not an asteroid (will add it to exclusion list)
05:52:01.06 +64:51:10.8 -- not an asteroid (will add it to exclusion list)
06:08:04.30 +56:49:58.5 -- not an asteroid (will add it to exclusion list)
05:55:54.78 +57:38:06.3 -- not an asteroid (will add it to exclusion list)
05:46:35.18 +63:18:35.9 -- not an asteroid (will add it to exclusion list)
05:44:53.17 +65:42:14.2 -- not an asteroid (will add it to exclusion list)
05:48:53.66 +64:03:09.8 -- not an asteroid (will add it to exclusion list)
05:55:17.18 +56:45:18.1 -- not an asteroid (will add it to exclusion list)
05:51:21.21 +65:21:31.9 -- not an asteroid (will add it to exclusion list)
06:02:54.00 +56:56:46.9 -- not an asteroid (will add it to exclusion list)
06:04:35.78 +57:23:54.7 -- not an asteroid (will add it to exclusion list)
07:14:41.40 +63:49:31.7 -- not an asteroid (will add it to exclusion list)
06:59:45.36 +57:30:10.5 -- not an asteroid (will add it to exclusion list)
07:08:26.21 +63:38:26.6 -- not an asteroid (will add it to exclusion list)
06:08:36.36 +64:07:57.5 -- not an asteroid (will add it to exclusion list)
05:48:53.89 +66:06:43.4 -- not an asteroid (will add it to exclusion list)
06:37:34.42 +62:19:25.8 -- not an asteroid (will add it to exclusion list)
06:19:48.85 +57:15:19.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:38:24.64 +65:46:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:17.37 +66:00:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:28.70 +66:09:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:37.56 +65:38:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:56.82 +65:44:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:58.40 +66:02:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:59.59 +65:34:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:01.02 +64:55:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:03.21 +64:30:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:03.60 +64:30:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:38.81 +63:52:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:49.25 +64:06:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:49.77 +64:25:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:21.66 +64:09:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:38.32 +65:21:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:43.82 +65:26:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:44.44 +64:38:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:53.17 +65:42:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:18.02 +62:19:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:35.64 +62:34:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:37.71 +63:15:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:42.88 +63:51:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.72 +65:53:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:56.54 +65:07:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:04.73 +65:59:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:27.83 +64:25:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:30.08 +64:46:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:35.18 +63:18:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:40.91 +65:49:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:07.84 +63:56:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:09.37 +65:06:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:43.75 +65:06:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:43.83 +65:46:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:08.13 +60:41:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:10.40 +66:01:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:21.35 +65:41:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:25.58 +63:43:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:38.89 +63:20:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:46.34 +65:49:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:51.89 +65:44:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.22 +63:58:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.66 +64:03:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.89 +66:06:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.92 +65:58:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.93 +60:10:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:20.22 +62:43:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:30.30 +63:19:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:33.21 +65:37:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:45.58 +65:56:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:59.24 +64:14:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:05.51 +66:07:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:14.18 +65:11:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:15.91 +61:27:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:16.33 +63:20:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:17.37 +63:47:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:24.85 +66:22:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:26.45 +65:03:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:32.44 +64:16:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:04.25 +63:52:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.08 +64:07:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:21.21 +65:21:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:29.11 +63:08:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:38.60 +65:02:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:47.53 +59:52:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:01.06 +64:51:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:03.90 +63:46:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:04.84 +58:38:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:10.92 +64:17:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:17.47 +60:03:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:26.91 +63:09:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:29.33 +63:09:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:38.74 +58:36:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:41.14 +65:33:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:42.43 +60:44:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:44.53 +63:42:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:53.12 +65:20:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.27 +59:24:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:14.24 +61:56:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:18.26 +61:26:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:19.26 +66:17:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:30.54 +65:20:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:48.84 +66:15:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:57.43 +64:35:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:14.98 +65:04:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:20.42 +65:52:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:35.49 +66:18:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:39.86 +61:58:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:49.11 +66:31:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:49.56 +63:46:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:17.18 +56:45:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:23.87 +65:12:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:23.95 +58:00:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:47.91 +64:54:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:54.78 +57:38:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:56.65 +64:29:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:01.74 +57:22:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:04.10 +65:55:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:13.16 +64:32:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:17.28 +66:10:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:18.99 +66:14:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:19.18 +56:48:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:29.09 +66:29:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:34.37 +59:18:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:36.66 +59:10:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:41.98 +59:24:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:48.35 +66:15:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:09.07 +57:09:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:16.53 +63:54:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:26.87 +57:25:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:15.79 +57:36:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:16.10 +65:30:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:18.11 +57:06:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:18.38 +57:54:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:19.46 +66:20:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:34.70 +59:04:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:43.00 +56:41:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:55.34 +60:24:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:45.25 +56:42:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:46.47 +61:04:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:51.56 +64:13:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:09.89 +57:00:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:27.28 +57:35:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:54.00 +56:56:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:52.87 +57:16:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:02.69 +59:32:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:35.78 +57:23:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:50.55 +66:41:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:32.40 +57:59:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:55.09 +66:06:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:04.30 +56:49:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:36.36 +64:07:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:06.93 +57:10:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:57.32 +60:41:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:47.33 +64:03:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:16.84 +59:12:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:48.85 +57:15:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.38 +58:25:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:34.42 +62:19:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:46.74 +59:52:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:04.96 +58:29:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:45.36 +57:30:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:26.21 +63:38:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:41.40 +63:49:31.7 -- 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)
05:38:24.64 +65:46:08.7 -- not a known variable star
05:39:17.37 +66:00:20.4 -- not a known variable star
05:39:28.70 +66:09:19.5 -- not a known variable star
05:39:37.56 +65:38:58.0 -- not a known variable star
05:39:56.82 +65:44:01.0 -- not a known variable star
05:39:58.40 +66:02:22.7 -- a known variable star
05:40:59.59 +65:34:37.5 -- not a known variable star
05:41:01.02 +64:55:13.4 -- not a known variable star
05:41:03.21 +64:30:02.1 -- not a known variable star
05:41:03.60 +64:30:14.8 -- not a known variable star
05:42:38.81 +63:52:35.2 -- not a known variable star
05:42:49.25 +64:06:54.4 -- not a known variable star
05:42:49.77 +64:25:14.5 -- a known variable star
05:43:21.66 +64:09:25.3 -- not a known variable star
05:43:38.32 +65:21:34.3 -- a known variable star
05:44:43.82 +65:26:08.8 -- not a known variable star
05:44:44.44 +64:38:45.3 -- not a known variable star
05:44:53.17 +65:42:14.2 -- not a known variable star
05:45:18.02 +62:19:01.1 -- not a known variable star
05:45:35.64 +62:34:30.8 -- a known variable star
05:45:37.71 +63:15:28.5 -- not a known variable star
05:45:42.88 +63:51:02.3 -- not a known variable star
05:45:50.72 +65:53:36.7 -- not a known variable star
05:45:56.54 +65:07:38.0 -- not a known variable star
05:46:04.73 +65:59:45.4 -- not a known variable star
05:46:27.83 +64:25:06.2 -- a known variable star
05:46:30.08 +64:46:41.0 -- not a known variable star
05:46:35.18 +63:18:35.9 -- a known variable star
05:46:40.91 +65:49:25.3 -- not a known variable star
05:47:07.84 +63:56:29.8 -- not a known variable star
05:47:09.37 +65:06:35.0 -- not a known variable star
05:47:43.75 +65:06:43.1 -- not a known variable star
05:47:43.83 +65:46:26.0 -- not a known variable star
05:48:08.13 +60:41:41.2 -- not a known variable star
05:48:10.40 +66:01:01.5 -- not a known variable star
05:48:21.35 +65:41:24.6 -- not a known variable star
05:48:25.58 +63:43:14.4 -- not a known variable star
05:48:38.89 +63:20:58.1 -- not a known variable star
05:48:46.34 +65:49:37.5 -- not a known variable star
05:48:51.89 +65:44:00.4 -- not a known variable star
05:48:53.22 +63:58:13.1 -- not a known variable star
05:48:53.66 +64:03:09.8 -- not a known variable star
05:48:53.89 +66:06:43.4 -- not a known variable star
05:48:53.92 +65:58:49.5 -- not a known variable star
05:49:06.93 +60:10:40.6 -- a known variable star
05:49:20.22 +62:43:51.2 -- not a known variable star
05:49:30.30 +63:19:37.7 -- a known variable star
05:49:33.21 +65:37:51.5 -- not a known variable star
05:49:45.58 +65:56:14.3 -- not a known variable star
05:49:59.24 +64:14:24.6 -- not a known variable star
05:50:05.51 +66:07:57.6 -- not a known variable star
05:50:14.18 +65:11:50.3 -- not a known variable star
05:50:15.91 +61:27:35.6 -- not a known variable star
05:50:16.33 +63:20:32.3 -- not a known variable star
05:50:17.37 +63:47:19.5 -- not a known variable star
05:50:24.85 +66:22:05.9 -- not a known variable star
05:50:26.45 +65:03:48.9 -- not a known variable star
05:50:32.44 +64:16:13.9 -- a known variable star
05:51:04.25 +63:52:24.3 -- not a known variable star
05:51:18.08 +64:07:02.4 -- not a known variable star
05:51:21.21 +65:21:31.9 -- not a known variable star
05:51:29.11 +63:08:01.1 -- a known variable star
05:51:38.60 +65:02:26.9 -- not a known variable star
05:51:47.53 +59:52:00.9 -- not a known variable star
05:52:01.06 +64:51:10.8 -- not a known variable star
05:52:03.90 +63:46:54.5 -- not a known variable star
05:52:04.84 +58:38:05.8 -- not a known variable star
05:52:10.92 +64:17:55.7 -- not a known variable star
05:52:17.47 +60:03:51.8 -- not a known variable star
05:52:26.91 +63:09:39.7 -- not a known variable star
05:52:29.33 +63:09:38.1 -- not a known variable star
05:52:38.74 +58:36:48.2 -- not a known variable star
05:52:41.14 +65:33:42.6 -- not a known variable star
05:52:42.43 +60:44:34.8 -- not a known variable star
05:52:44.53 +63:42:44.0 -- not a known variable star
05:52:53.12 +65:20:49.6 -- not a known variable star
05:53:06.27 +59:24:32.4 -- not a known variable star
05:53:14.24 +61:56:44.3 -- not a known variable star
05:53:18.26 +61:26:49.6 -- not a known variable star
05:53:19.26 +66:17:40.9 -- not a known variable star
05:53:30.54 +65:20:10.2 -- not a known variable star
05:53:48.84 +66:15:04.4 -- a known variable star
05:53:57.43 +64:35:48.4 -- not a known variable star
05:54:14.98 +65:04:06.9 -- not a known variable star
05:54:20.42 +65:52:35.2 -- not a known variable star
05:54:35.49 +66:18:21.9 -- not a known variable star
05:54:39.86 +61:58:47.2 -- not a known variable star
05:54:49.11 +66:31:53.0 -- not a known variable star
05:54:49.56 +63:46:24.3 -- not a known variable star
05:55:17.18 +56:45:18.1 -- a known variable star
05:55:23.87 +65:12:34.8 -- not a known variable star
05:55:23.95 +58:00:33.0 -- not a known variable star
05:55:47.91 +64:54:56.9 -- not a known variable star
05:55:54.78 +57:38:06.3 -- not a known variable star
05:55:56.65 +64:29:48.6 -- not a known variable star
05:56:01.74 +57:22:49.0 -- not a known variable star
05:56:04.10 +65:55:08.6 -- not a known variable star
05:56:13.16 +64:32:17.8 -- not a known variable star
05:56:17.28 +66:10:13.0 -- not a known variable star
05:56:18.99 +66:14:51.5 -- not a known variable star
05:56:19.18 +56:48:39.3 -- not a known variable star
05:56:29.09 +66:29:22.0 -- not a known variable star
05:56:34.37 +59:18:10.5 -- not a known variable star
05:56:36.66 +59:10:44.8 -- not a known variable star
05:56:41.98 +59:24:23.7 -- not a known variable star
05:56:48.35 +66:15:45.9 -- not a known variable star
05:57:09.07 +57:09:59.9 -- not a known variable star
05:57:16.53 +63:54:56.9 -- not a known variable star
05:57:26.87 +57:25:23.9 -- not a known variable star
05:58:15.79 +57:36:17.7 -- a known variable star
05:58:16.10 +65:30:13.1 -- not a known variable star
05:58:18.11 +57:06:15.9 -- not a known variable star
05:58:18.38 +57:54:01.6 -- not a known variable star
05:58:19.46 +66:20:38.6 -- not a known variable star
05:58:34.70 +59:04:15.6 -- a known variable star
05:58:43.00 +56:41:18.7 -- not a known variable star
05:58:55.34 +60:24:53.8 -- not a known variable star
05:59:45.25 +56:42:01.6 -- a known variable star
05:59:46.47 +61:04:53.4 -- a known variable star
05:59:51.56 +64:13:05.2 -- not a known variable star
06:00:09.89 +57:00:13.6 -- a known variable star
06:02:27.28 +57:35:01.1 -- not a known variable star
06:02:54.00 +56:56:46.9 -- not a known variable star
06:03:52.87 +57:16:15.7 -- not a known variable star
06:04:02.69 +59:32:22.3 -- a known variable star
06:04:35.78 +57:23:54.7 -- not a known variable star
06:04:50.55 +66:41:30.9 -- not a known variable star
06:05:32.40 +57:59:30.5 -- not a known variable star
06:06:55.09 +66:06:35.7 -- not a known variable star
06:08:04.30 +56:49:58.5 -- not a known variable star
06:08:36.36 +64:07:57.5 -- a known variable star
06:10:06.93 +57:10:09.0 -- not a known variable star
06:10:57.32 +60:41:12.7 -- not a known variable star
06:14:47.33 +64:03:15.6 -- not a known variable star
06:16:16.84 +59:12:35.5 -- a known variable star
06:19:48.85 +57:15:19.1 -- a known variable star
06:25:49.38 +58:25:42.5 -- not a known variable star
06:37:34.42 +62:19:25.8 -- a known variable star
06:40:46.74 +59:52:04.1 -- a known variable star
06:58:04.96 +58:29:17.2 -- a known variable star
06:59:45.36 +57:30:10.5 -- a known variable star
07:08:26.21 +63:38:26.6 -- a known variable star
07:14:41.40 +63:49:31.7 -- not a known variable star
Found 117 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
143 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)2461083.99311642 -observatory 500
22:43:15.81 -08:36:38.9 Mercury (-1.1mag)
22:18:56.99 -12:02:56.2 Venus (-3.9mag)
21:12:41.21 -17:14:58.2 Mars (1.1mag)
07:09:00.09 +22:48:52.9 Jupiter (-2.6mag)
00:01:28.19 -02:11:09.3 Saturn (1.0mag)
03:39:31.77 +19:20:00.4 Uranus (5.7mag)
00:02:30.52 -01:09:25.7 Neptune (7.8mag)
20:27:53.39 -23:02:32.0 Pluto (14.6mag)
17:40:22.88 -28:23:30.4 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Feb 12 06:12 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461083.99311642:
07:08:51.91 +22:49:06.3 Io (5.3mag)
07:09:04.95 +22:48:38.8 Europa (5.5mag)
07:08:46.06 +22:49:12.5 Ganymede (4.9mag)
07:09:00.06 +22:48:40.1 Callisto (6.0mag)
07:11:18.15 +23:09:07.6 Himalia (15.0mag)
07:08:53.95 +22:49:03.7 Thebe (15.8mag)
07:10:55.22 +23:11:59.5 Elara (17.0mag)
07:04:06.56 +24:01:51.4 Pasiphae (17.0mag)
07:18:01.19 +22:33:50.8 Carme (18.0mag)
00:01:22.76 -02:10:48.9 Titan (8.7mag)
00:01:30.84 -02:11:07.1 Rhea (10.1mag)
00:01:03.67 -02:12:53.0 Iapetus (11.5mag)
00:01:30.11 -02:10:54.3 Hyperion (14.7mag)
00:03:34.10 -01:57:45.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 12 06:12 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461083.99311642:
07:41:37.34 +23:00:19.4 JWST
17:17:02.45 +42:20:49.1 Chandra
18:23:14.66 -17:47:06.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 12 06:12 spacecraft.txt
############################################################
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)2461083.99311642 at 500
16:41:05.44 -10:51:39.9 17.7mag 10P/Tempel
03:29:05.16 +28:26:34.8 18.1mag 123P/West-Hartley
20:48:41.94 -10:07:05.1 22.4mag 141P/Machholz
01:00:04.41 +09:08:40.7 17.6mag 145P/Shoemaker-Levy 5
11:11:49.13 +29:19:14.1 17.8mag 164P/Christensen
09:38:39.51 -34:07:38.4 18.0mag 195P/Hill
15:51:04.51 -07:24:38.0 18.5mag 210P/Christensen
17:31:19.80 -21:38:45.6 17.4mag 218P/LINEAR
16:04:20.60 -18:17:31.4 15.2mag 235P/LINEAR
03:43:37.22 +25:53:42.1 17.5mag 240P/NEAT
15:03:12.17 +07:29:03.3 14.6mag 24P/Schaumasse
23:54:43.52 +04:21:30.4 18.1mag 261P/Larson
11:27:11.43 -03:35:33.4 17.4mag 29P/Schwassmann-Wachmann 1
01:07:26.22 +01:27:19.9 18.9mag 302P/Lemmon-PanSTARRS
07:06:33.25 +27:17:27.8 19.7mag 407P/PanSTARRS-Fuls
16:50:13.45 -11:18:47.0 17.5mag 40P/Vaisala 1
11:08:03.39 -09:15:38.0 16.6mag 43P/Wolf-Harrington
13:22:55.46 -05:09:04.6 19.4mag 489P/Denning
04:28:09.45 +49:23:35.0 17.7mag 493P/2024 Q2 (LONEOS)
06:02:39.13 +49:15:28.7 17.8mag 63P/Wild 1
22:55:35.28 -03:51:14.0 16.3mag 78P/Gehrels 2
19:25:10.74 -23:27:41.2 15.1mag 88P/Howell
15:22:12.06 -28:11:50.9 18.7mag P/2023 S1 (PanSTARRS)
04:43:14.69 -73:08:28.2 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:37.35 +31:11:11.0 18.1mag C/2017 K2 (PanSTARRS)
20:00:56.98 -64:56:31.8 18.1mag C/2020 V2 (ZTF)
17:17:12.32 +03:23:05.4 16.3mag C/2021 G2 (ATLAS)
22:45:53.89 +28:36:18.0 16.8mag C/2022 E2 (ATLAS)
03:28:28.75 +24:26:45.4 15.7mag C/2022 N2 (PANSTARRS)
09:11:46.67 +28:58:45.8 15.3mag C/2022 QE78 (ATLAS)
08:38:51.41 -07:42:59.5 16.6mag C/2022 R6 (PanSTARRS)
23:40:58.88 +48:06:58.8 17.9mag C/2023 C2 (ATLAS)
10:01:55.73 -22:03:58.4 17.5mag C/2023 F3 (ATLAS)
20:14:31.36 +61:17:08.0 17.2mag C/2023 H5 (Lemmon)
19:32:57.76 -03:17:55.3 16.1mag C/2023 R1 (PANSTARRS)
02:46:00.81 +35:46:59.5 18.5mag C/2023 RS61 (PanSTARRS)
20:43:59.17 +81:15:28.8 18.0mag C/2023 X2 (Lemmon)
06:55:03.35 +63:26:12.6 17.2mag C/2024 A1 (ATLAS)
00:33:01.45 -36:38:19.8 10.8mag C/2024 E1 (Wierzchos)
11:52:13.76 -04:20:23.6 18.1mag C/2024 G2 (ATLAS)
19:18:49.53 +00:21:38.1 19.0mag C/2024 G4 (PanSTARRS)
16:36:59.82 -02:55:02.0 17.8mag C/2024 G6 (ATLAS)
19:46:38.52 +01:33:23.8 15.6mag C/2024 J3 (ATLAS)
02:42:36.69 -33:24:29.2 15.4mag C/2024 T5 (ATLAS)
16:45:59.90 -54:26:46.5 15.3mag C/2025 A6 (Lemmon)
04:55:01.99 +66:08:13.3 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)
16:01:06.83 -20:02:40.4 15.0mag C/2025 L1 (ATLAS)
02:12:50.09 -17:39:28.7 16.7mag C/2025 Q3 (ATLAS)
01:57:11.95 +16:20:47.8 20.8mag C/2025 R2 (SWAN)
22:17:30.89 +17:32:35.8 16.8mag C/2025 R3 (PANSTARRS)
21:35:28.63 -14:44:06.8 20.4mag C/2025 T1 (ATLAS)
03:30:27.74 -25:02:36.2 17.4mag C/2026 A1 (MAPS)
20:26:44.02 +16:22:00.2 16.6mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.7K Feb 12 06:13 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 06:12 asassn_transients_list.txt
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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 06:12 tocp_transients_list.txt