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_215304_TTUQ2b1x1_10693_QTkiYAQO
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.6167,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1167 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:00.82 -00:39:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 11.63 06:54:38.70 -05:59:05.2
218.62509 -2.01476 galactic Mon Second-epoch detections are separated by 1.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.6658-05.9908 | 06:54:39.82 -05:59:19.4 (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 J103.6658-05.9908,2461129.6167,11.63,0.05,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
ATO J103.6658-05.9908 20260330.1167 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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:38.70 -05:59:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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,2461129.6167,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260330.1167 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:30.57 -01:04:43.5 ;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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 11.65 06:34:14.65 -04:53:32.3
215.34381 -6.04737 galactic Mon Second-epoch detections are separated by 0.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3103538282851408512 | 06:34:12.51 -04:53:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103538282851408512,2461129.6167,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103538282851408512 20260330.1167 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:14.65 -04:53:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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 3102509487863923328,2461129.6167,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102509487863923328 20260330.1167 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:28.16 -04:07:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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 3102097995636478720,2461129.6167,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102097995636478720 20260330.1167 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:44.64 -04:35:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 11.97 07:06:54.14 -01:17:15.9
215.84386 2.85134 galactic Mon Second-epoch detections are separated by 2.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109498293007726848 | 07:06:54.85 -01:17:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109498293007726848,2461129.6167,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109498293007726848 20260330.1167 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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:06:54.14 -01:17:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 12.00 06:50:29.90 -00:35:54.8
213.35753 -0.48198 galactic Mon Second-epoch detections are separated by 5.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 J102.6262-00.5898,2461129.6167,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.6262-00.5898 20260330.1167 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:50:29.90 -00:35:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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,2461129.6167,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1167 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:00.68 -02:52:21.6 ;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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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 3113345346754410112,2461129.6167,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113345346754410112 20260330.1167 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:28.86 -00:00:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 12.27 06:43:50.38 +01:35:50.8
210.64379 -0.96135 galactic Mon Second-epoch detections are separated by 4.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.9580+01.5948 | 06:43:50.38 +01:35:50.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461129.6167,12.27,0.05,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
ATO J100.9580+01.5948 20260330.1167 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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:50.38 +01:35:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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 3106074070200575616,2461129.6167,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106074070200575616 20260330.1167 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:07.56 -01:52:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 12.39 06:47:03.95 -03:46:19.9
215.79375 -2.69042 galactic Mon Second-epoch detections are separated by 1.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105398626463066368 | 06:47:06.49 -03:46:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 295449
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105398626463066368,2461129.6167,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105398626463066368 20260330.1167 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:03.95 -03:46:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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
GDS_J0641591-011108,2461129.6167,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0641591-011108 20260330.1167 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:59.17 -01:11:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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
WY Mon,2461129.6167,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WY Mon 20260330.1167 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:42.53 -04:56:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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
ASASSN-V J063753.27-055523.1,2461129.6167,12.30,0.05,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
ASASSN-V J063753.27-055523.1 20260330.1167 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/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:53.34 -05:55:17.4 ;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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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,2461129.6167,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0801 Mon 20260330.1167 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:01.68 -04:35:39.6 ;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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1167 2461129.6167 10.45 06:55:01.07 -01:02:19.1
214.26440 0.32278 galactic Mon Second-epoch detections are separated by 3.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.7675-01.0334 | 06:55:02.28 -01:02:02.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2V 1956ApJS....2..271M LF 9 -01 315
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.7675-01.0334,2461129.6167,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7675-01.0334 20260330.1167 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:55:01.07 -01:02:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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_21-48-24_20_00sec_-10_00C_LIGHT_0064_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_21-47-18_20_00sec_-10_00C_LIGHT_0063_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: 2461129.61706575 30.03.2026 02:48:24.481 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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: 7 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): 29389
Objects passed selection criteria: 29233
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: 20526
Average stars matched: 19474 (94.8748 %)
Memory usage VmPeak: 133496 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 21:55:31 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: 2461129.61706575 30.03.2026 02:48:24.481 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 166
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: 60 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): 212839
Objects passed selection criteria: 212210
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: 152474
Average stars matched: 143494 (94.1106 %)
Memory usage VmPeak: 1966360 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 22:01:04 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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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: 2461129.61630595
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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits'
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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 06:51:24.634 -02:00:46.23
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 06:51:21.866 -02:00:14.80
Angular distance between the image centers 0.09 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 06:51:24.634 -02:00:46.23
Second-epoch second image center 06:51:21.866 -02:00:14.80
Angular distance between the image centers 0.01446 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.924t5GtgWO
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.8WIDLk151g
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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits &> /tmp/tmp.xsrUMcuO1Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits &> /tmp/tmp.9AP1ZE8s1s
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
2.7 pix fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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.924t5GtgWO (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_215304_TTUQ2b1x1_10693_QTkiYAQO/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.8WIDLk151g (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_215304_TTUQ2b1x1_10693_QTkiYAQO/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.xsrUMcuO1Z (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_215304_TTUQ2b1x1_10693_QTkiYAQO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=897, passed=12561
Got 12561 stars (including 11652 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 12561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.1'
Seting catalog search parameters based on the expected field of view 923.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012821 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010257 (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 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: 2.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.02"
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 683 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.92"
Estimated accuracy of the plate solution: 1.92"
Excluding outliers - 635 stars left (next iteration limit 650)
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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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.9AP1ZE8s1s (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_215304_TTUQ2b1x1_10693_QTkiYAQO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=907, passed=12662
Got 12662 stars (including 11746 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 12662 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.6'
Seting catalog search parameters based on the expected field of view 921.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012800 (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 0.010240 (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 646 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: 2.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.10"
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: 3.03"
Estimated accuracy of the plate solution: 2.14"
Excluding outliers - 623 stars left (next iteration limit 633)
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_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/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_215304_TTUQ2b1x1_10693_QTkiYAQO/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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53264_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 53264_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (67.4") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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 06:51:24.634 -02:00:46.23
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 06:51:21.866 -02:00:14.80
Angular distance between the image centers 0.09 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 06:51:24.634 -02:00:46.23
Second-epoch second image center 06:51:21.866 -02:00:14.80
Angular distance between the image centers 0.01446 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.WCVsVwNOk1
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.DnM0KJfy91
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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits &> /tmp/tmp.wAi6rQYAoz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits &> /tmp/tmp.q2A5enn1lR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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 139 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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
12.9 mag. fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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.WCVsVwNOk1 (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_215304_TTUQ2b1x1_10693_QTkiYAQO/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.DnM0KJfy91 (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_215304_TTUQ2b1x1_10693_QTkiYAQO/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.wAi6rQYAoz (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_215304_TTUQ2b1x1_10693_QTkiYAQO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=7638, passed=91632
Got 91632 stars (including 83905 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 91632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 923.1'
Seting catalog search parameters based on the expected field of view 923.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012821 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010257 (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 625 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: 2.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.93"
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 642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.92"
Estimated accuracy of the plate solution: 1.98"
Excluding outliers - 592 stars left (next iteration limit 605)
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_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.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.q2A5enn1lR (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_215304_TTUQ2b1x1_10693_QTkiYAQO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-02-Q2b1x1_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=7757, passed=92996
Got 92996 stars (including 85151 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 92996 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.6'
Seting catalog search parameters based on the expected field of view 921.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012800 (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 0.010240 (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: 2.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 639 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.41"
Estimated accuracy of the plate solution: 2.09"
Excluding outliers - 583 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_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits -region wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/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_215304_TTUQ2b1x1_10693_QTkiYAQO/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_21-47-18_20.00sec_-10.00C_LIGHT_0063.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_215304_TTUQ2b1x1_10693_QTkiYAQO/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-47-18_20.00sec_-10.00C_LIGHT_0063.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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_215304_TTUQ2b1x1_10693_QTkiYAQO/wcs_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064.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__out285093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out154583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57802.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): 29s
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: 10s
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Considering the candidate 285084_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285084_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (67.0") between the two second-epoch detections
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Considering the candidate 285086_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 285086_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 285093_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285093_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:51:02.62 +01:07:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.989 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285094_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285094_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (38.3") between the two second-epoch detections
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Considering the candidate 285099_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285099_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (75.4") between the two second-epoch detections
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Considering the candidate 285102_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285102_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:54:08.05 -05:53:01.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 285106_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285106_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:53:54.42 +00:53:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.533 3113971690424905728 103.47724737496 +00.88351500760 12.1834 11.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285107_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285107_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (86.1") between the two second-epoch detections
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Considering the candidate 285108_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285108_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:52:13.80 -00:19:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.234 3113277073955197952 103.05718640970 -00.32225778318 12.6390 11.8315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285110_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285110_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 285111_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285111_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 285113_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285113_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 285118_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285118_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (46.7") between the two second-epoch detections
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Considering the candidate 285121_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285121_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (140.5") between the two second-epoch detections
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Considering the candidate 285122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 285124_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285124_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 285125_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285125_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
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Considering the candidate 285126_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285126_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (66.6") between the two second-epoch detections
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Considering the candidate 285127_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285127_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (103.6") between the two second-epoch detections
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Considering the candidate 285129_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285129_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (89.4") between the two second-epoch detections
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Considering the candidate 285130_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285130_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (69.1") between the two second-epoch detections
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Considering the candidate 285131_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285131_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
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Considering the candidate 285135_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285135_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (62.5") between the two second-epoch detections
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Considering the candidate 285139_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285139_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (34.0") between the two second-epoch detections
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Considering the candidate 285140_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 285140_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 285141_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285141_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 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 285144_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285144_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (49.3") between the two second-epoch detections
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Considering the candidate 285147_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285147_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (47.1") between the two second-epoch detections
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Considering the candidate 285148_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285148_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (57.6") between the two second-epoch detections
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Considering the candidate 285149_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285149_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:53:11.52 -01:33:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.164 3112276892032630400 103.29879130350 -01.56062176551 12.3437 11.9261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285152_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285152_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (67.0") between the two second-epoch detections
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Considering the candidate 285153_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285153_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (68.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285155_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285155_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 285156_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285156_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (75.3") between the two second-epoch detections
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Considering the candidate 285157_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285157_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:51:45.76 +00:30:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.019 3113577137549962752 102.94011496702 +00.50292634664 12.0373 11.7992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 285158_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285158_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (88.6") between the two second-epoch detections
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Considering the candidate 285163_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285163_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (30.5") between the two second-epoch detections
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Considering the candidate 285165_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285165_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (65.3") between the two second-epoch detections
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Considering the candidate 285167_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 285167_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (70.8") between the two second-epoch detections
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Considering the candidate 288010_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 288010_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:50:40.22 -00:32:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 2.267 3113219246514568576 102.66724852826 -00.54000569020 11.1991 10.5064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288108_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 288108_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (78.9") between the two second-epoch detections
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Considering the candidate 288952_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 288952_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (44.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289120_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 289120_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:51:39.78 +00:25:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 1.446 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289792_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 289792_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290057_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290057_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (43.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290398_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290398_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (38.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290466_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290466_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (63.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290484_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290484_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (48.6") between the two second-epoch detections
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Considering the candidate 290504_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290504_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (106.2") between the two second-epoch detections
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Considering the candidate 290548_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290548_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:54:00.71 -04:24:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 3.485 3102117237090175232 103.50202616480 -04.40275734180 12.3382 12.0757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290655_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 290655_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:32:18.50 -05:51:42.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291077_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 291077_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (62.7") between the two second-epoch detections
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Considering the candidate 291120_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 291120_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:50:41.66 -00:33:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.172 3113219001708838656 102.67311151201 -00.56248734381 12.4370 12.0693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291316_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 291316_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (53.1") between the two second-epoch detections
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Considering the candidate 291425_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 291425_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (104.8") between the two second-epoch detections
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Considering the candidate 292088_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292088_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:36:41.10 -05:13:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 292122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:52:25.40 -05:17:26.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 292260_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292260_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 292357_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292357_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (45.1") between the two second-epoch detections
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Considering the candidate 292469_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292469_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (153.0") between the two second-epoch detections
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Considering the candidate 292663_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292663_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (78.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292684_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 292684_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292930_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 292930_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292972_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292972_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (157.6") between the two second-epoch detections
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Considering the candidate 292988_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 292988_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:51:21.43 -03:31:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.576 3102793677260019072 102.83948079787 -03.52496786001 12.7794 12.2627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293103_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293103_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (37.2") between the two second-epoch detections
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Considering the candidate 293208_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293208_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (36.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293245_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293245_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293302_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293302_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293310_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293310_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (57.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293409_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293409_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (108.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293499_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293499_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (107.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293677_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293677_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:53:08.05 -04:35:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.918 3102106791729894272 103.28369873380 -04.59861811590 12.6605 12.1037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293819_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293819_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (45.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293920_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293920_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293946_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293946_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:43:32.72 -01:21:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.669 3107239586888081920 100.88566983865 -01.35610698240 12.4804 11.6457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293962_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 293962_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (75.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294339_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 294339_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294590_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 294590_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294777_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 294777_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (87.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294824_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 294824_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294952_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 294952_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295083_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295083_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295151_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295151_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295182_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295182_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (66.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295184_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 295184_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295258_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295258_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (61.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295380_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295380_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (48.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295490_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295490_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (52.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295549_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295549_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (52.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295582_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295582_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (75.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295594_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295594_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:50:44.50 -00:31:38.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295614_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295614_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (59.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295732_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 295732_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295735_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295735_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (88.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295754_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295754_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (65.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295760_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295760_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (74.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295792_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295792_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (44.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295832_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 295832_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296036_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296036_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296125_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296125_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (51.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296201_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296201_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:44:33.65 -01:39:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.938 3107031126354300032 101.14073851257 -01.66087173871 12.8835 12.1345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296248_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296248_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (64.8") between the two second-epoch detections
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Considering the candidate 296483_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296483_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:37:58.52 -01:25:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.067 3118919183510887040 099.49400345973 -01.42388158330 12.8781 12.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296681_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296681_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (151.7") between the two second-epoch detections
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Considering the candidate 296742_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296742_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 296762_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296762_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (31.8") between the two second-epoch detections
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Considering the candidate 296789_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296789_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (73.9") between the two second-epoch detections
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Considering the candidate 296804_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296804_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:54:09.26 -05:52:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 296914_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 296914_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (45.6") between the two second-epoch detections
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Considering the candidate 297010_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297010_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:54:30.24 -04:07:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.835 3102509449203351296 103.62527411825 -04.12544889351 12.9516 12.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297043_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297043_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (70.7") between the two second-epoch detections
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Considering the candidate 297046_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297046_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 297053_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 297053_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 297255_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297255_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:45:00.17 -00:03:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.049 3107483197430678400 101.25075565208 -00.05928951009 13.0563 12.7107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297287_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 297287_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 297301_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297301_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (60.8") between the two second-epoch detections
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Considering the candidate 297523_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 297523_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (54.4") between the two second-epoch detections
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Considering the candidate 297550_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 297550_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 298047_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298047_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:40:00.93 -03:20:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.278 3106367983402590976 100.00447557547 -03.34879787013 13.2694 12.4475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298117_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298117_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (65.7") between the two second-epoch detections
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Considering the candidate 298130_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298130_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (57.9") between the two second-epoch detections
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Considering the candidate 298328_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298328_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (59.0") between the two second-epoch detections
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Considering the candidate 298367_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 298367_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 298382_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298382_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:54:14.81 -05:59:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 5.343 3101066172693925120 103.56296805322 -05.99249014951 13.3393 12.8732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298684_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298684_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (37.7") between the two second-epoch detections
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Considering the candidate 298969_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 298969_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:52:57.58 -03:05:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.886 3105839461908787584 103.23885232014 -03.08364397921 13.4535 12.9348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 299009_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 299009_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (44.8") between the two second-epoch detections
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Considering the candidate 299066_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 299066_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (38.6") between the two second-epoch detections
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Considering the candidate 299112_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 299112_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:51:42.24 +00:25:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.654 3113575453922853632 102.92527875821 +00.42011914305 13.6376 13.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 154583_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 131156_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 131156_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 57802_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 57802_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 31804_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 65114_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 65114_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 228912_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
**** FOUND 06:50:00.76 +01:46:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 2.393 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 158645_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
Preparing report for the candidate 158645_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 121122_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (67.0") between the two second-epoch detections
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064
The candidate 199360_fd_Mon-02-Q2b1x1_2026-03-29_21-48-24_20.00sec_-10.00C_LIGHT_0064 did not pass the final checks