This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62
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 03 30.1156 2461129.6156 12.33 06:46:12.98 +00:51:06.4
211.57850 -0.77320 galactic Mon Second-epoch detections are separated by 8.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.5447+00.8442 | 06:46:12.98 +00:51:06.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A8V 2012A&A...541A..34S CoRoT 102807727
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.5447+00.8442,2461129.6156,12.33,0.05,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
ATO J101.5447+00.8442 20260330.1156 12.33CV 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:46:12.98 +00:51:06.4 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.12 06:51:44.60 +00:29:57.8
212.52228 0.29566 galactic Mon Second-epoch detections are separated by 3.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113577137549962752 | 06:51:45.63 +00:30:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.052 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113577137549962752,2461129.6156,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113577137549962752 20260330.1156 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:44.60 +00:29:57.8 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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
CD Mon,2461129.6156,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260330.1156 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:30.69 -01:04:44.6 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.38 06:54:00.84 -04:24:12.5
217.14500 -1.43462 galactic Mon Second-epoch detections are separated by 4.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.4965-04.3935 | 06:54:00.49 -04:24:09.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V 2012A&A...541A..34S CoRoT 110696985
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.4965-04.3935,2461129.6156,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4965-04.3935 20260330.1156 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:00.84 -04:24:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.38 06:53:39.59 +01:30:56.8
211.83595 1.18536 galactic Mon Second-epoch detections are separated by 2.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.4115+01.5116 | 06:53:37.37 +01:30:24.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.076 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4115+01.5116,2461129.6156,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4115+01.5116 20260330.1156 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:39.59 +01:30:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.78 06:51:21.58 -03:31:29.7
216.06098 -1.62389 galactic Mon Second-epoch detections are separated by 6.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.8381-03.5210 | 06:51:21.58 -03:31:29.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2.5IVa 2012A&A...543A.125G CoRoT 110753571 J-Ks=0.353+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8381-03.5210,2461129.6156,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8381-03.5210 20260330.1156 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:21.58 -03:31:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.63 06:34:14.69 -04:53:34.1
215.34433 -6.04745 galactic Mon Second-epoch detections are separated by 4.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3103538282851408512 | 06:34:12.51 -04:53:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103538282851408512,2461129.6156,11.63,0.05,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 3103538282851408512 20260330.1156 11.63CV 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:14.69 -04:53:34.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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 3102097995636478720,2461129.6156,12.03,0.05,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 3102097995636478720 20260330.1156 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:44.71 -04:35:32.4 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 11.97 06:51:05.06 -02:56:38.4
215.51230 -1.42054 galactic Mon Second-epoch detections are separated by 4.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.7735-02.9489 | 06:51:05.06 -02:56:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7IIIa 2012A&A...543A.125G CoRoT 103019472
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.7735-02.9489,2461129.6156,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7735-02.9489 20260330.1156 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:05.06 -02:56:38.4 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 12.01 06:50:29.73 -00:35:57.9
213.35797 -0.48300 galactic Mon Second-epoch detections are separated by 6.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.6262-00.5898 | 06:50:30.27 -00:35:57.0 (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 J102.6262-00.5898,2461129.6156,12.01,0.05,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
ATO J102.6262-00.5898 20260330.1156 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:50:29.73 -00:35:57.9 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 12.21 07:01:26.08 -05:15:54.9
218.75581 -0.18333 galactic Mon Second-epoch detections are separated by 8.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101401523743429248 | 07:01:25.52 -05:16:15.2 (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 3101401523743429248,2461129.6156,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101401523743429248 20260330.1156 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:26.08 -05:15:54.9 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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,2461129.6156,12.11,0.05,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
target 20260330.1156 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:21.22 -05:21:27.0 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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,2461129.6156,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1156 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:44.90 -04:29:33.8 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 12.30 06:56:45.78 +00:46:05.9
212.85506 1.53511 galactic Mon Second-epoch detections are separated by 7.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.2021+00.7657 | 06:56:45.78 +00:46:05.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.162+/-0.038 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2021+00.7657,2461129.6156,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2021+00.7657 20260330.1156 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:45.78 +00:46:05.9 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1156 2461129.6156 12.29 06:52:01.74 -04:08:55.0
216.69258 -1.75916 galactic Mon Second-epoch detections are separated by 7.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.0073-04.1482 | 06:52:03.63 -04:08:30.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F4V 2012A&A...543A.125G CoRoT 110678224 J-Ks=0.310+/-0.037 (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
ATO J103.0073-04.1482,2461129.6156,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0073-04.1482 20260330.1156 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:52:01.74 -04:08:55.0 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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 3105249642638290688,2461129.6156,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105249642638290688 20260330.1156 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:17.55 -04:35:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0801 Mon,2461129.6156,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0801 Mon 20260330.1156 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:01.78 -04:35:41.0 ;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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20_00sec_-10_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20_00sec_-10_00C_LIGHT_0061_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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461129.61594306 30.03.2026 02:46:47.480 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 29371
Objects passed selection criteria: 29211
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 20426.2
Average stars matched: 19382.5 (94.8902 %)
Memory usage VmPeak: 133500 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:51:28 CDT 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461129.61594306 30.03.2026 02:46:47.480 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 145
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 52 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): 212734
Objects passed selection criteria: 212089
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 151991
Average stars matched: 143048 (94.1161 %)
Memory usage VmPeak: 2228504 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:56:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> '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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.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: 2461129.61525339
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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits'
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.614 -02:00:14.84
Angular distance between the image centers 0.08 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.637 -02:00:46.26
Angular distance between the image centers 0.08 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 06:51:24.614 -02:00:14.84
Second-epoch second image center 06:51:24.637 -02:00:46.26
Angular distance between the image centers 0.00873 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.Fps3a40Mhb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.Jo9ZyzVa4A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits &> /tmp/tmp.E5g963k9S4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits &> /tmp/tmp.28yt8P9qNp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Fps3a40Mhb (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 457 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: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 16.11"
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 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 16.01"
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.Jo9ZyzVa4A (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 73 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: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.E5g963k9S4 (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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=905, passed=12397
Got 12397 stars (including 11480 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 12397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.5'
Seting catalog search parameters based on the expected field of view 921.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012799 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010239 (36.9 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 649 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: 2.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.19"
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 673 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.11"
Estimated accuracy of the plate solution: 2.10"
Excluding outliers - 624 stars left (next iteration limit 634)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.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.28yt8P9qNp (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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=894, passed=12449
Got 12449 stars (including 11544 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 12449 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 662 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: 2.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.82"
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 702 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.75"
Estimated accuracy of the plate solution: 1.97"
Excluding outliers - 651 stars left (next iteration limit 667)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.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
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53211_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 53211_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (105.5") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Mon-02-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 ####
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.614 -02:00:14.84
Angular distance between the image centers 0.08 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.637 -02:00:46.26
Angular distance between the image centers 0.08 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 06:51:24.614 -02:00:14.84
Second-epoch second image center 06:51:24.637 -02:00:46.26
Angular distance between the image centers 0.00873 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.U9z8xPy9Yf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.nJAhahWUDu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits &> /tmp/tmp.ldvyixnnYS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits &> /tmp/tmp.LlEnhNDJVA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 121 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
12.9 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
12.9 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.U9z8xPy9Yf (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.43"
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 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 7.42"
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.nJAhahWUDu (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 68 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: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ldvyixnnYS (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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=7411, passed=90937
Got 90937 stars (including 83438 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 90937 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.5'
Seting catalog search parameters based on the expected field of view 921.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012799 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010239 (36.9 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 615 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: 3.05"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.25"
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 643 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.24"
Estimated accuracy of the plate solution: 2.22"
Excluding outliers - 591 stars left (next iteration limit 597)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.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.LlEnhNDJVA (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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.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_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=7579, passed=91727
Got 91727 stars (including 84055 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 91727 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 632 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: 2.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.82"
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 675 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.82"
Estimated accuracy of the plate solution: 1.99"
Excluding outliers - 629 stars left (next iteration limit 630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.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
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-45-47_20.00sec_-10.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_214902_TTUQ2b1x1_8580_yVJ4gz62/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out285082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65114.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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 285082_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 285082_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 285093_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285093_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 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 285097_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285097_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (228.4") between the two second-epoch detections
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Considering the candidate 285103_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285103_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (94.2") between the two second-epoch detections
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Considering the candidate 285111_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285111_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (114.5") between the two second-epoch detections
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Considering the candidate 285118_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285118_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:52:13.87 -00:19:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.203 3113277073955197952 103.05718640970 -00.32225778318 12.6390 11.8315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285120_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285120_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (111.4") between the two second-epoch detections
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Considering the candidate 285125_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285125_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:51:02.71 +01:07:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 5.361 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285129_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285129_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (106.1") between the two second-epoch detections
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Considering the candidate 285134_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285134_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (119.5") between the two second-epoch detections
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Considering the candidate 285138_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285138_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (87.7") between the two second-epoch detections
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Considering the candidate 285139_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285139_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (80.8") between the two second-epoch detections
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Considering the candidate 285141_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285141_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 285143_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285143_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:54:08.11 -05:53:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 285144_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285144_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (200.3") between the two second-epoch detections
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Considering the candidate 285151_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285151_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 285153_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285153_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (113.9") between the two second-epoch detections
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Considering the candidate 285154_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285154_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (149.7") between the two second-epoch detections
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Considering the candidate 285156_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285156_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (106.3") between the two second-epoch detections
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Considering the candidate 285160_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285160_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 285161_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285161_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (118.2") between the two second-epoch detections
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Considering the candidate 285162_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285162_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (40.8") between the two second-epoch detections
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Considering the candidate 285164_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285164_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (117.2") between the two second-epoch detections
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Considering the candidate 285165_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285165_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 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 285166_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285166_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (103.1") between the two second-epoch detections
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Considering the candidate 285167_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285167_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (83.7") between the two second-epoch detections
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Considering the candidate 285172_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 285172_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 285175_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285175_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (38.2") between the two second-epoch detections
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Considering the candidate 285177_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 285177_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:38:08.50 -01:28:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.06, MAG_FAINT_SEARCH_LIMIT=11.04)GAIADR2_OUTPUT=# 2.378 3106909218001458560 099.53605034664 -01.47152094130 11.0094 10.4057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 287428_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 287428_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (173.5") between the two second-epoch detections
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Considering the candidate 288160_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 288160_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (66.7") between the two second-epoch detections
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Considering the candidate 289246_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 289246_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (54.6") between the two second-epoch detections
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Considering the candidate 289301_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 289301_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:51:39.80 +00:25:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.489 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289869_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 289869_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 290219_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 290219_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (53.9") between the two second-epoch detections
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Considering the candidate 290223_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 290223_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 290243_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 290243_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (59.4") between the two second-epoch detections
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Considering the candidate 290321_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 290321_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 290569_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 290569_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 291153_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 291153_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:50:41.74 -00:33:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.971 3113219001708838656 102.67311151201 -00.56248734381 12.4370 12.0693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291312_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 291312_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (135.6") between the two second-epoch detections
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Considering the candidate 291774_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 291774_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (99.0") between the two second-epoch detections
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Considering the candidate 292184_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292184_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (154.5") between the two second-epoch detections
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Considering the candidate 292207_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292207_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (171.6") between the two second-epoch detections
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Considering the candidate 292306_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292306_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (104.5") between the two second-epoch detections
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Considering the candidate 292327_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292327_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:52:25.52 -05:17:28.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 292359_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292359_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (63.6") between the two second-epoch detections
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Considering the candidate 292573_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292573_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (137.7") between the two second-epoch detections
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Considering the candidate 292585_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 292585_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 292917_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 292917_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 292944_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 292944_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (174.4") between the two second-epoch detections
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Considering the candidate 293017_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293017_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
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Considering the candidate 293101_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293101_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (41.9") between the two second-epoch detections
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Considering the candidate 293252_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293252_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:53:08.20 -04:35:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.688 3102106791729894272 103.28369873380 -04.59861811590 12.6605 12.1037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293310_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293310_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (130.9") between the two second-epoch detections
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Considering the candidate 293437_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293437_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:36:41.14 -05:13:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293509_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293509_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (94.9") between the two second-epoch detections
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Considering the candidate 293621_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293621_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (152.5") between the two second-epoch detections
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Considering the candidate 293651_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293651_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:43:32.79 -01:21:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.439 3107239586888081920 100.88566983865 -01.35610698240 12.4804 11.6457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293702_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293702_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (101.2") between the two second-epoch detections
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Considering the candidate 293782_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293782_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 293893_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293893_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (48.3") between the two second-epoch detections
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Considering the candidate 293904_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 293904_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (41.4") between the two second-epoch detections
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Considering the candidate 294142_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294142_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:44:24.26 -00:05:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 4.220 3119491028336256768 101.09994003962 -00.09532438243 12.7782 12.1362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294316_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294316_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (86.2") between the two second-epoch detections
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Considering the candidate 294509_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294509_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (110.7") between the two second-epoch detections
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Considering the candidate 294517_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 294517_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 294557_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 294557_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 294826_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294826_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (99.7") between the two second-epoch detections
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Considering the candidate 294829_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294829_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 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 294935_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 294935_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (105.8") between the two second-epoch detections
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Considering the candidate 295073_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295073_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (175.1") between the two second-epoch detections
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Considering the candidate 295106_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 295106_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 295167_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295167_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (91.1") between the two second-epoch detections
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Considering the candidate 295181_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295181_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:56:49.35 -03:40:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 4.318 3102647025594892928 104.20463857527 -03.67195383887 12.9220 12.3828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295294_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295294_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (149.8") between the two second-epoch detections
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Considering the candidate 295729_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295729_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (75.9") between the two second-epoch detections
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Considering the candidate 295793_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295793_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:50:44.56 -00:31:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 295857_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295857_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 295886_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295886_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (119.3") between the two second-epoch detections
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Considering the candidate 295945_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295945_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (117.7") between the two second-epoch detections
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Considering the candidate 295954_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295954_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (72.9") between the two second-epoch detections
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Considering the candidate 295989_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 295989_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:54:30.26 -04:07:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.410 3102509449203351296 103.62527411825 -04.12544889351 12.9516 12.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296004_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296004_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (121.1") between the two second-epoch detections
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Considering the candidate 296007_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296007_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (106.6") between the two second-epoch detections
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Considering the candidate 296125_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296125_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 296172_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296172_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:44:33.86 -01:39:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.770 3107031126354300032 101.14073851257 -01.66087173871 12.8835 12.1345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296261_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296261_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:35:16.44 -04:45:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 2.736 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296313_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296313_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:54:09.34 -05:52:28.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 296370_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 296370_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 296400_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296400_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:37:58.59 -01:25:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.516 3118919183510887040 099.49400345973 -01.42388158330 12.8781 12.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296457_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 296457_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 296698_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296698_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (111.2") between the two second-epoch detections
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Considering the candidate 296797_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296797_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (34.9") between the two second-epoch detections
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Considering the candidate 296902_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296902_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (154.5") between the two second-epoch detections
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Considering the candidate 296908_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 296908_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:45:00.35 -00:03:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.568 3107483197430678400 101.25075565208 -00.05928951009 13.0563 12.7107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297084_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 297084_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 297140_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297140_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 297213_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297213_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 297480_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 297480_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 297642_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 297642_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297662_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297662_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (62.3") between the two second-epoch detections
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Considering the candidate 297674_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297674_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 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 297683_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297683_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (39.8") between the two second-epoch detections
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Considering the candidate 297789_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297789_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (38.4") between the two second-epoch detections
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Considering the candidate 297857_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297857_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (101.0") between the two second-epoch detections
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Considering the candidate 297936_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 297936_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (134.3") between the two second-epoch detections
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Considering the candidate 298049_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 298049_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 298251_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 298251_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 298280_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 298280_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (51.6") between the two second-epoch detections
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Considering the candidate 298292_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 298292_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 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 298570_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 298570_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:52:44.07 -02:03:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.165 3106065480266043520 103.18305627524 -02.05733531426 13.2692 12.3177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298637_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 298637_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 228912_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
**** FOUND 06:50:00.90 +01:46:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 4.618 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 122073_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 122073_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (31.7") between the two second-epoch detections
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Considering the candidate 231205_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 231205_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 131156_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 131156_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (111.0") between the two second-epoch detections
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Considering the candidate 65114_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
Preparing report for the candidate 65114_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
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Considering the candidate 40418_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 40418_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 121122_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (107.9") between the two second-epoch detections
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062
The candidate 199360_fd_Mon-02-Q2b1x1_2026-03-29_21-46-47_20.00sec_-10.00C_LIGHT_0062 did not pass the final checks