This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0804 Oph,2461126.9044,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0804 Oph 20260327.4044 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:01.65 +07:55:11.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_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,2461126.9044,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4044 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:40:13.38 +08:07:41.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_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,2461126.9044,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4044 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:18:52.94 +07:39:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_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,2461126.9044,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4044 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:24:03.65 +07:36:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4044 2461126.9044 13.01 17:42:45.12 +09:41:48.4
33.97860 19.62135 galactic Oph Second-epoch detections are separated by 4.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:42:45.12 +09:41:48.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=1.656+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9044,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4044 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:42:45.12 +09:41:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4044 2461126.9044 13.07 18:04:53.09 +05:38:17.8
32.69078 12.91293 galactic Oph Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J271.2270+05.6494 | 18:04:53.09 +05:38:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J271.2270+05.6494,2461126.9044,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J271.2270+05.6494 20260327.4044 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:04:53.09 +05:38:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4044 2461126.9044 13.22 17:41:50.56 +10:03:40.5
34.22630 19.98007 galactic Oph Second-epoch detections are separated by 2.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J265.4586+10.0597 | 17:41:50.56 +10:03:40.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J265.4586+10.0597,2461126.9044,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J265.4586+10.0597 20260327.4044 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:41:50.56 +10:03:40.5 ;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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_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
V0425 Oph,2461126.9044,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0425 Oph 20260327.4044 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:26.47 +06:59:04.9 ;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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20_00sec_-15_00C_LIGHT_0434_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20_00sec_-15_00C_LIGHT_0433_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: 2461093.97799654 22.02.2026 11:28:08.901 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
First image: 2461093.97799654 22.02.2026 11:28:08.901 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Last image: 2461126.90470590 27.03.2026 09:42:36.590 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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.: -7.86
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16086
Objects passed selection criteria: 16050
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 14495.5
Average stars matched: 14171 (97.7614 %)
Memory usage VmPeak: 122340 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 05:57:01 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: 2461093.97799654 22.02.2026 11:28:08.901 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
First image: 2461093.97799654 22.02.2026 11:28:08.901 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Last image: 2461126.90470590 27.03.2026 09:42:36.590 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 41 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): 139030
Objects passed selection criteria: 138755
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 110509
Average stars matched: 106452 (96.3288 %)
Memory usage VmPeak: 1974136 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 05:59:53 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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
SExtractor catalog cache: saved Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat to cache
SExtractor catalog cache: saved Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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: 2461126.90412586
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits exists and is non-empty
Saving wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits to local_wcs_cache/
'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits' -> 'local_wcs_cache/wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits'
wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits exists and is non-empty
Saving wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits to local_wcs_cache/
'wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits' -> 'local_wcs_cache/wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits'
wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits exists and is non-empty
Saving wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits to local_wcs_cache/
'wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits' -> 'local_wcs_cache/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits'
wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits exists and is non-empty
Saving wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits to local_wcs_cache/
'wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits' -> 'local_wcs_cache/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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 18:00:22.904 +05:59:32.25
Second-epoch image center 18:00:01.090 +06:00:20.46
Angular distance between the image centers 0.09 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 18:00:22.904 +05:59:32.25
Second-epoch image center 18:00:01.686 +05:59:40.66
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:00:01.090 +06:00:20.46
Second-epoch second image center 18:00:01.686 +05:59:40.66
Angular distance between the image centers 0.01133 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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits &> /tmp/tmp.lXQENILDJO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits &> /tmp/tmp.U0FJShsFCf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits &> /tmp/tmp.8YpRvjOOgo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits &> /tmp/tmp.XkKUcHJhN5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
Found non-empty wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
The reference image (wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits) and catalog (wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat) found
'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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 11256 out of 21117 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.903286
a=0.000000 b=1.000000 c=22.903286
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
2.3 pix Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
3.5 pix fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
3.7 pix fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Limiting magnitude estimates:
15.0 mag. Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
15.0 mag. Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
14.4 mag. fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
14.4 mag. fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.8 (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.lXQENILDJO (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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits' -> 'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS_IMAGE_NAME=wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS-calibrated image found: wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Checking if the catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits alredy exist and is non-empty...
Catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS catalog name: wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1735, passed=21117
Got 21117 stars (including 19354 good ones) from the SExtractor catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
util/solve_plate_with_UCAC5 got 21117 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 921 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits -region wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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.U0FJShsFCf (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/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits' -> 'wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS_IMAGE_NAME=wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS-calibrated image found: wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Checking if the catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits alredy exist and is non-empty...
Catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS catalog name: wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1700, passed=20958
Got 20958 stars (including 19237 good ones) from the SExtractor catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat
util/solve_plate_with_UCAC5 got 20958 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 920 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits -region wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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.8YpRvjOOgo (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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS_IMAGE_NAME=wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS-calibrated image found: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Checking if the catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS catalog name: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=704, passed=14272
Got 14272 stars (including 13563 good ones) from the SExtractor catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat
util/solve_plate_with_UCAC5 got 14272 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 915 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits -region wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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.XkKUcHJhN5 (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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=688, passed=13870
Got 13870 stars (including 13175 good ones) from the SExtractor catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat
util/solve_plate_with_UCAC5 got 13870 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 914 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits -region wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits'
Saving fully-calibrated image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits'
Saving fully-calibrated image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits'
Saving fully-calibrated image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits'
Preparing the HTML report for the field Oph-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out03017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31280.dat to exclusion_list_gaiadr2.txt
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 31204_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 31204_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:05:25.83 +05:13:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31231_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 31231_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:24:07.55 +05:11:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31280_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 31280_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:58:16.75 +04:20:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.624 4469783941102781440 269.56985043919 +04.33678138958 11.7948 11.0693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15299_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 15299_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:18.31 +08:44:02.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06147_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 06147_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:00:15.85 +04:22:10.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04754_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 04754_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:16:36.85 +03:41:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03017_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 03017_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:05:04.50 +02:46:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 2.174 4468581148401631104 271.26905339899 +02.76986639988 10.6373 8.9425 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07321_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 07321_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:19:14.71 +04:56:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16972_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 16972_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:20.87 +09:33:52.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06354_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 06354_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:43:28.64 +04:34:09.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02742_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 02742_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:47:53.63 +02:42:28.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Oph-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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
SExtractor catalog cache: saved Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat to cache
SExtractor catalog cache: saved Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Creating symlink local_wcs_cache/wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits exists and is non-empty
wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits exists and is non-empty
wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits exists and is non-empty
wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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 18:00:22.904 +05:59:32.25
Second-epoch image center 18:00:01.090 +06:00:20.46
Angular distance between the image centers 0.09 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 18:00:22.904 +05:59:32.25
Second-epoch image center 18:00:01.686 +05:59:40.66
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:00:01.090 +06:00:20.46
Second-epoch second image center 18:00:01.686 +05:59:40.66
Angular distance between the image centers 0.01133 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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits &> /tmp/tmp.fJ33pT0HrN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits &> /tmp/tmp.WyoOpBK2Uz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits &> /tmp/tmp.bFhar2toX1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits &> /tmp/tmp.nseWUsb4BK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
Found non-empty wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits and wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
The reference image (wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits) and catalog (wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat) found
'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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 11804 out of 173688 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.738842
a=0.000000 b=1.000000 c=22.738842
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 61 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
2.0 pix Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
3.7 pix fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
3.8 pix fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Limiting magnitude estimates:
15.2 mag. Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
15.2 mag. Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
14.5 mag. fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
14.4 mag. fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fJ33pT0HrN (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/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits' -> 'wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS_IMAGE_NAME=wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS-calibrated image found: wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Checking if the catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits alredy exist and is non-empty...
Catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
WCS catalog name: wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=19164, passed=173661
Got 173661 stars (including 154271 good ones) from the SExtractor catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat
util/solve_plate_with_UCAC5 got 173661 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 924 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.35"
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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits -region wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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.WyoOpBK2Uz (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/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits' -> 'wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS_IMAGE_NAME=wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS-calibrated image found: wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Checking if the catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits alredy exist and is non-empty...
Catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat corresponding to the image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
WCS catalog name: wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=19443, passed=175914
Got 175914 stars (including 156223 good ones) from the SExtractor catalog wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat
util/solve_plate_with_UCAC5 got 175914 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 918 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits -region wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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.bFhar2toX1 (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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS_IMAGE_NAME=wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS-calibrated image found: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Checking if the catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
WCS catalog name: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=8232, passed=80537
Got 80537 stars (including 72246 good ones) from the SExtractor catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat
util/solve_plate_with_UCAC5 got 80537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 918 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits -region wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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.nseWUsb4BK (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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat corresponding to the image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=8205, passed=77387
Got 77387 stars (including 69131 good ones) from the SExtractor catalog wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat
util/solve_plate_with_UCAC5 got 77387 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 918 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits -region wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits
Saving fully-calibrated image wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_Oph-03-Q2b1x1_2026-02-22_05-29-04_20.00sec_-15.00C_LIGHT_0564.fits
Saving fully-calibrated image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-41-46_20.00sec_-15.00C_LIGHT_0433.fits
Saving fully-calibrated image wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.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_Oph-03-Q2b1x1_055337_TTUQ2b1x1_21744_1373HNfk/wcs_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434.fits
Preparing the HTML report for the field Oph-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out199122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out104583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79563.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 199122_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199122_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:47.25 +04:56:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.646 4471200700496471296 271.94535884766 +04.93903303840 13.7022 12.9781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199125_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199125_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:35:33.29 +07:50:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.160 4487369259495122048 263.88778963295 +07.83995475362 13.2142 12.3938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199132_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199132_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:12:34.79 +08:02:33.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 199133_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199133_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:15.75 +01:59:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.496 4468202534145958400 271.81623799338 +01.99867551521 12.9803 12.1484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199138_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199138_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:49:01.34 +06:44:13.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 199140_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 199140_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 199141_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199141_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:47:19.95 +03:07:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.111 4472173355967233792 266.83230151900 +03.12770602456 12.9835 12.0601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199142_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199142_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:03:57.52 +04:25:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.521 4471241141905685120 270.98894252867 +04.42571532619 13.2391 12.4681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199143_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 199143_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 199145_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 199145_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 199149_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199149_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:23:27.05 +04:44:26.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 199151_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 199151_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 199157_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199157_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:24:08.57 +08:28:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.639 4478505164259020672 276.03537276597 +08.46830240440 12.4052 11.2808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199160_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199160_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:54:02.49 +09:54:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 199161_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 199161_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 199162_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199162_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:20:10.95 +08:20:56.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 199397_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199397_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:19:10.62 +07:17:20.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 199470_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199470_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:21:30.54 +05:24:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 199532_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 199532_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:37:31.40 +03:27:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110263_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 110263_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:19:09.33 +07:15:35.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31085_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 31085_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:47:53.61 +02:42:28.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 25456_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 25456_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:05:27.63 +02:29:32.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 138251_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 138251_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:18.29 +08:44:02.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33733_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 33733_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:00:38.76 +02:55:57.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 58877_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 58877_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:00:15.85 +04:22:09.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44899_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 44899_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:16:36.84 +03:41:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66360_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 66360_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:19:14.74 +04:56:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70783_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 70783_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:24:07.56 +05:11:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140083_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 140083_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:17:45.24 +08:39:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79563_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 79563_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 98938_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 98938_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:18:48.74 +06:41:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136861_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 136861_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:18:52.65 +08:51:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72127_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 72127_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:05:25.83 +05:13:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48320_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 48320_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:44:47.60 +03:52:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44661_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 44661_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:33:10.57 +03:36:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27742_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 27742_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:05:04.40 +02:46:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166399_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 166399_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 137496_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 137496_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:43:33.02 +08:42:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80853_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 80853_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:17:56.39 +05:44:21.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 34170_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 34170_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:34:10.87 +03:03:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104583_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
Preparing report for the candidate 104583_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
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Considering the candidate 93473_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 93473_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:00:52.88 +06:16:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101565_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 101565_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:51:00.80 +06:46:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98865_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 98865_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:56:56.01 +06:29:17.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 90963_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 90963_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:53:14.03 +06:06:08.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 61314_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 61314_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:52:00.05 +04:29:15.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 47254_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 47254_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:54:28.38 +03:43:56.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 50976_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 50976_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:09:33.86 +03:59:37.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 48743_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 48743_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:48:20.34 +03:48:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 34767_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 34767_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:09:53.94 +03:07:08.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 39635_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 39635_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:10:40.23 +03:19:29.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17580_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 17580_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:49:19.05 +01:57:44.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15779_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 15779_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:04:37.26 +01:55:05.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173224_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 173224_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:07:20.86 +09:33:51.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 66036_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 66036_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:43:28.64 +04:34:09.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 96165_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 96165_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:41:32.46 +06:18:48.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18914_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 18914_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:39:08.58 +02:01:41.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76990_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 76990_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 18:21:28.41 +05:26:08.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 27201_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 27201_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:44:34.69 +02:34:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 123694_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 123694_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks
**** FOUND 17:34:36.66 +09:35:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22743_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434
The candidate 22743_fd_Oph-03-Q2b1x1_2026-03-27_04-42-36_20.00sec_-15.00C_LIGHT_0434 did not pass the final checks