This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.4335 2461126.9335 12.76 20:57:18.86 +24:28:19.9
69.94854 -13.53132 galactic Vul Second-epoch detections are separated by 7.8" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3287+24.4688 | 20:57:17.95 +24:28:26.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.3287+24.4688,2461126.9335,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.3287+24.4688 20260327.4335 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:18.86 +24:28:19.9 ;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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4335 2461126.9335 12.60 21:30:19.97 +23:02:36.5
73.99080 -20.17629 galactic Peg Second-epoch detections are separated by 0.8" and 1.0 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 1797242160368586624 | 21:30:19.10 +23:02:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1797242160368586624,2461126.9335,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1797242160368586624 20260327.4335 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:19.97 +23:02:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4335 2461126.9335 12.43 21:29:51.77 +23:36:14.7
74.34686 -19.71380 galactic Peg Second-epoch detections are separated by 1.9" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1797345583181254784 | 21:29:51.42 +23:36:10.1 (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 1797345583181254784,2461126.9335,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1797345583181254784 20260327.4335 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:51.77 +23:36:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4335 2461126.9335 12.89 21:15:22.64 +21:47:52.1
70.56332 -18.43451 galactic Vul Second-epoch detections are separated by 2.3" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:15:22.64 +21:47:52.1 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9335,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4335 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:15:22.64 +21:47:52.1 ;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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_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,2461126.9335,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4335 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:50.21 +26:04:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2104312+204253,2461126.9335,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2104312+204253 20260327.4335 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:31.32 +20:42:54.8 ;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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_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
V0382 Peg,2461126.9335,12.09,0.05,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
V0382 Peg 20260327.4335 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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:55.93 +23:13:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_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
ASAS J212353+2025.7,2461126.9335,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J212353+2025.7 20260327.4335 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:53.27 +20:25:52.2 ;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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20_00sec_-15_00C_LIGHT_0477_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: 2461036.54561373 27.12.2025 01:05:31.026 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461036.54561373 27.12.2025 01:05:31.026 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461126.93375971 27.03.2026 10:24:26.839 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.99
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: 4 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): 15225
Objects passed selection criteria: 15139
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 10940.8
Average stars matched: 10236.2 (93.5608 %)
Memory usage VmPeak: 120004 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 Fri Mar 27 05:43:33 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: 2461036.54561373 27.12.2025 01:05:31.026 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461036.54561373 27.12.2025 01:05:31.026 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461126.93375971 27.03.2026 10:24:26.839 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 105
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 24 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): 107666
Objects passed selection criteria: 107329
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: 75097.5
Average stars matched: 70133.8 (93.3903 %)
Memory usage VmPeak: 1876648 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 Fri Mar 27 05:45:34 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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
SExtractor catalog cache: saved Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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: 2461126.93325263
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits'
wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits'
wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits exists and is non-empty
Saving wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits to local_wcs_cache/
'wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits'
wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:13:51.296 +21:59:55.63
Second-epoch image center 21:13:49.179 +21:57:27.23
Angular distance between the image centers 0.04 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 21:13:51.296 +21:59:55.63
Second-epoch image center 21:13:48.840 +21:57:24.36
Angular distance between the image centers 0.04 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 21:13:49.179 +21:57:27.23
Second-epoch second image center 21:13:48.840 +21:57:24.36
Angular distance between the image centers 0.00153 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00153 deg. (min. required shift: 0.00164 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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.LnNfq52XZK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.hGbsI0kiAI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits &> /tmp/tmp.1M6yDbUZBU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.XYNxY6WHrA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
Found non-empty wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
The reference image (wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat) found
'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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 12381 out of 18556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929726
a=0.000000 b=1.000000 c=22.929726
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
2.4 pix Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
4.3 pix fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
4.1 pix fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Limiting magnitude estimates:
14.9 mag. Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
14.9 mag. Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
13.7 mag. fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
13.8 mag. fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LnNfq52XZK (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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1581, passed=18556
Got 18556 stars (including 16957 good ones) from the SExtractor catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
util/solve_plate_with_UCAC5 got 18556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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.hGbsI0kiAI (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/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1543, passed=18535
Got 18535 stars (including 16975 good ones) from the SExtractor catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat
util/solve_plate_with_UCAC5 got 18535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 913.8'
Seting catalog search parameters based on the expected field of view 913.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012692 (45.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010153 (36.6 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 514 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.10"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.36"
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 526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.25"
Estimated accuracy of the plate solution: 1.52"
Excluding outliers - 474 stars left (next iteration limit 512)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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.1M6yDbUZBU (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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS-calibrated image found: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Checking if the catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=310, passed=8335
Got 8335 stars (including 8022 good ones) from the SExtractor catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 8335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 929 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits -region wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.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.XYNxY6WHrA (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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=309, passed=8434
Got 8434 stars (including 8122 good ones) from the SExtractor catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 8434 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 927 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: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits'
Saving fully-calibrated image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits'
Saving fully-calibrated image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits'
Saving fully-calibrated image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits'
Preparing the HTML report for the field Vul-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 21037_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 21037_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:02:07.14 +18:10:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21880_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 21880_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:28:52.46 +22:09:35.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13265_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 13265_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:22:05.63 +19:48:22.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20325_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 20325_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:57:44.84 +20:03:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17151_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 17151_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:29:22.85 +18:10:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14947_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 14947_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:13:01.14 +18:56:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06506_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 06506_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:21:04.94 +23:51:21.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09258_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 09258_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:28:59.75 +22:10:48.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09289_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 09289_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:58:16.57 +22:19:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06688_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 06688_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:29:56.88 +23:38:21.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14216_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 14216_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:00:27.83 +19:19:49.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vul-03-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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
SExtractor catalog cache: saved Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits exists and is non-empty
wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:13:51.296 +21:59:55.63
Second-epoch image center 21:13:49.179 +21:57:27.23
Angular distance between the image centers 0.04 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 21:13:51.296 +21:59:55.63
Second-epoch image center 21:13:48.840 +21:57:24.36
Angular distance between the image centers 0.04 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 21:13:49.179 +21:57:27.23
Second-epoch second image center 21:13:48.840 +21:57:24.36
Angular distance between the image centers 0.00153 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00153 deg. (min. required shift: 0.00164 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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.3wbUWec4sZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.WVrzNVNkFv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits &> /tmp/tmp.4mJw3S7XIN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.AzvxmLXGLm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
Found non-empty wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
The reference image (wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat) found
'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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 13465 out of 136126 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.751440
a=0.000000 b=1.000000 c=22.751440
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
2.2 pix Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
4.2 pix fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
4.1 pix fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Limiting magnitude estimates:
15.1 mag. Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
15.1 mag. Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
13.8 mag. fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
13.8 mag. fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.1 (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.3wbUWec4sZ (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/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=14038, passed=136076
Got 136076 stars (including 121801 good ones) from the SExtractor catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat
util/solve_plate_with_UCAC5 got 136076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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.WVrzNVNkFv (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/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=13978, passed=135637
Got 135637 stars (including 121417 good ones) from the SExtractor catalog wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat
util/solve_plate_with_UCAC5 got 135637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 913.8'
Seting catalog search parameters based on the expected field of view 913.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012692 (45.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010153 (36.6 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 524 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: 2.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.00"
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 537 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.98"
Estimated accuracy of the plate solution: 1.47"
Excluding outliers - 483 stars left (next iteration limit 515)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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.4mJw3S7XIN (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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS-calibrated image found: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Checking if the catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3355, passed=43290
Got 43290 stars (including 39902 good ones) from the SExtractor catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 43290 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 931 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: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits -region wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.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.AzvxmLXGLm (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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3118, passed=43723
Got 43723 stars (including 40573 good ones) from the SExtractor catalog wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 43723 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 928 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: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_Vul-03-Q2b1x1_2025-12-26_19-05-31_20.00sec_-14.90C_LIGHT_0006.fits
Saving fully-calibrated image wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_Vul-03-Q2b1x1_2025-12-26_19-06-11_20.00sec_-15.00C_LIGHT_0007.fits
Saving fully-calibrated image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-23-43_20.00sec_-15.00C_LIGHT_0477.fits
Saving fully-calibrated image wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.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_2026-03-27_CI_Vul-03-Q2b1x1_053543_TTUQ2b1x1_9232_VhMITLqY/wcs_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478.fits
Preparing the HTML report for the field Vul-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out156213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out135142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99728.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 156198_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 156198_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 156212_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 156212_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 156213_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 156213_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:18:55.98 +24:31:54.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 156216_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 156216_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 156219_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 156219_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 156222_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 156222_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:58:02.44 +17:49:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 5.159 1765139337120558720 314.50890524527 +17.82483753498 12.4728 11.7954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158447_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 158447_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 158471_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 158471_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 158541_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 158541_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:50:10.91 +21:13:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160148_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 160148_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:29:10.27 +22:10:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160383_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 160383_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 161023_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 161023_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 161087_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 161087_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 161204_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 161204_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:00:20.02 +19:20:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161867_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 161867_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 161929_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 161929_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:30:08.94 +23:56:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162238_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162238_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:54:05.75 +19:44:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162408_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162408_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:21:06.44 +24:21:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162539_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162539_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 162854_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162854_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:24:03.06 +24:15:05.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 162864_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162864_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 162972_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 162972_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163119_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163119_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:32:37.33 +24:11:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163176_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163176_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163255_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163255_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:23:30.69 +24:57:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163382_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163382_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163492_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 163492_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 163493_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163493_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163508_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163508_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163575_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163575_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163610_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163610_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163662_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163662_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163742_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163742_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 163841_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163841_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:26:27.75 +21:53:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163952_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 163952_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164042_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164042_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164065_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164065_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164431_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164431_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164467_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164467_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164478_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164478_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164506_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164506_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164527_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164527_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164657_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164657_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164677_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164677_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164746_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164746_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164817_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164817_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164906_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164906_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164954_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164954_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164955_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164955_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164970_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164970_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 164971_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 164971_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 46559_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 46559_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:29:56.90 +23:38:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 125941_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 125941_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:22:05.63 +19:48:22.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 102015_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 102015_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:02:07.14 +18:10:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103651_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 103651_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:29:22.79 +18:10:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79516_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 79516_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:12:31.94 +21:29:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81793_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 81793_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 14418_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 14418_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 128763_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 128763_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:57:44.87 +20:03:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99728_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 99728_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 107733_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 107733_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:10:17.37 +18:34:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55399_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 55399_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 135142_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
Preparing report for the candidate 135142_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
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Considering the candidate 148386_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 148386_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:23:19.51 +23:28:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147881_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 147881_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:49:31.02 +23:34:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53411_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 53411_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:53:00.28 +23:22:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53239_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 53239_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:58:25.12 +23:30:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113196_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 113196_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:13:01.14 +18:56:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65878_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 65878_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:10:31.78 +22:27:22.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70993_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 70993_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:20:14.13 +22:01:36.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45144_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 45144_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:21:04.94 +23:51:20.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44304_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 44304_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:03:29.79 +23:59:50.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 39120_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 39120_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:23:59.14 +24:16:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67127_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 67127_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:28:59.76 +22:10:48.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67539_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 67539_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 20:58:16.59 +22:19:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120474_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 120474_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:26:26.83 +19:22:35.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25288_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 25288_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:24:07.55 +25:18:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117581_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 117581_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:00:27.85 +19:19:49.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12951_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 12951_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:24:34.14 +26:10:30.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99758_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 99758_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:28:59.86 +17:54:22.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20702_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 20702_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
**** FOUND 21:38:45.26 +25:29:57.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134793_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478
The candidate 134793_fd_Vul-03-Q2b1x1_2026-03-27_05-24-26_20.00sec_-15.00C_LIGHT_0478 did not pass the final checks
