This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 22.1893 2461121.6893 12.23 04:17:00.51 +45:17:03.8
156.37028 -3.82455 galactic Per Second-epoch detections are separated by 0.6" 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 J064.2556+45.2818 | 04:16:58.94 +45:17:12.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.1893* 04 17 00.51 +45 17 03.8 12.2 U Per 9 0
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 J064.2556+45.2818,2461121.6893,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J064.2556+45.2818 20260322.1893 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:00.51 +45:17:03.8 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_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!
TCP 2026 03 22.1893* 03 32 32.27 +41 26 30.6 9.8 U Per 9 0
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
V0513 Per,2461121.6893,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0513 Per 20260322.1893 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:32.27 +41:26:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_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!
TCP 2026 03 22.1893* 03 26 57.50 +41 04 00.2 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.6893,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.1893 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:57.50 +41:04:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.1893 2461121.6893 12.01 02:55:33.55 +40:50:36.6
146.88943 -16.18350 galactic Per Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J043.8895+40.8436 | 02:55:33.50 +40:50:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.262+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.1893* 02 55 33.55 +40 50 36.6 12.0 U Per 9 0
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 J043.8895+40.8436,2461121.6893,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J043.8895+40.8436 20260322.1893 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:33.55 +40:50:36.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.1893 2461121.6893 12.82 02:53:14.01 +43:05:08.8
145.39774 -14.41020 galactic Per Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:53:14.01 +43:05:08.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.763+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.1893* 02 53 14.01 +43 05 08.8 12.8 U Per 9 0
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,2461121.6893,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260322.1893 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:53:14.01 +43:05:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_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!
TCP 2026 03 22.1893* 03 26 17.64 +50 35 46.0 13.3 U Per 9 0
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
BG Per,2461121.6893,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
BG Per 20260322.1893 13.32CV 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:17.64 +50:35:46.0 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.1893 2461121.6893 12.19 02:55:27.84 +40:54:33.8
146.84022 -16.13419 galactic Per Second-epoch detections are separated by 3.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J043.8770+40.9067 | 02:55:27.66 +40:54:33.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.954+/-0.028 (M)
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!
TCP 2026 03 22.1893* 02 55 27.84 +40 54 33.8 12.2 U Per 9 0
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 J043.8770+40.9067,2461121.6893,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J043.8770+40.9067 20260322.1893 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:27.84 +40:54:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.77657470 23.12.2025 06:38:06.054 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
First image: 2461032.77657470 23.12.2025 06:38:06.054 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Last image: 2461121.68969434 22.03.2026 04:32:59.591 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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): 23340
Objects passed selection criteria: 23306
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 20836
Average stars matched: 20442.2 (98.1102 %)
Memory usage VmPeak: 127672 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 Sat Mar 21 23:39:07 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.77657470 23.12.2025 06:38:06.054 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
First image: 2461032.77657470 23.12.2025 06:38:06.054 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Last image: 2461121.68969434 22.03.2026 04:32:59.591 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 166
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 52 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 155602
Objects passed selection criteria: 155329
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 135871
Average stars matched: 131761 (96.9751 %)
Memory usage VmPeak: 1922768 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 Sat Mar 21 23:41:36 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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: 2461121.68891523
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits exists and is non-empty
Saving wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits to local_wcs_cache/
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits' -> 'local_wcs_cache/wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits'
wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits exists and is non-empty
Saving wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits to local_wcs_cache/
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits' -> 'local_wcs_cache/wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits'
wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits'
wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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 03:35:59.356 +45:59:56.12
Second-epoch image center 03:36:00.406 +46:00:08.59
Angular distance between the image centers 0.00 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 03:35:59.356 +45:59:56.12
Second-epoch image center 03:35:59.722 +45:59:30.65
Angular distance between the image centers 0.01 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 03:36:00.406 +46:00:08.59
Second-epoch second image center 03:35:59.722 +45:59:30.65
Angular distance between the image centers 0.01072 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits &> /tmp/tmp.nbpq9kP4wa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits &> /tmp/tmp.OPTubieyMW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits &> /tmp/tmp.L7mnrHpEt5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits &> /tmp/tmp.8pAC9AilUy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
Found non-empty wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
The reference image (wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits) and catalog (wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat) found
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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 9218 out of 24873 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.961870
a=0.000000 b=1.000000 c=22.961870
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
2.1 pix Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
2.5 pix fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
2.6 pix fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.3 mag. Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
15.3 mag. Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
14.8 mag. fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
14.8 mag. fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nbpq9kP4wa (6) ############
Parsing command line arguments...
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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits' -> 'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2376, passed=24873
Got 24873 stars (including 22468 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 24873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 970 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits -region wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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.OPTubieyMW (6) ############
Parsing command line arguments...
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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits' -> 'wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2373, passed=24808
Got 24808 stars (including 22415 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat
util/solve_plate_with_UCAC5 got 24808 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 971 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits -region wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.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.L7mnrHpEt5 (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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1138, passed=17121
Got 17121 stars (including 15967 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 17121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 973 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits -region wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.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.8pAC9AilUy (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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1122, passed=16990
Got 16990 stars (including 15855 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 16990 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 973 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits -region wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits'
Saving fully-calibrated image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits'
Preparing the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31513.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31491_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31491_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:59:56.40 +42:37:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31502_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31502_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:14:56.24 +48:49:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31508_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31508_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:36.48 +42:54:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31513_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 31513_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31514_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31514_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:11.68 +40:52:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.943 336115207053011840 043.54762021339 +40.88278955100 12.0101 11.5257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31524_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31524_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:42:34.76 +50:15:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31529_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 31529_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:41:50.84 +41:59:16.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05394_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 05394_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:23.17 +48:39:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21459_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 21459_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:32:32.27 +41:26:30.6
04:17:00.51 +45:17:03.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Creating symlink local_wcs_cache/wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits exists and is non-empty
wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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 03:35:59.356 +45:59:56.12
Second-epoch image center 03:36:00.406 +46:00:08.59
Angular distance between the image centers 0.00 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 03:35:59.356 +45:59:56.12
Second-epoch image center 03:35:59.722 +45:59:30.65
Angular distance between the image centers 0.01 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 03:36:00.406 +46:00:08.59
Second-epoch second image center 03:35:59.722 +45:59:30.65
Angular distance between the image centers 0.01072 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits &> /tmp/tmp.l9BVGj9JDp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits &> /tmp/tmp.ZKKiQC4Aqs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits &> /tmp/tmp.mVuxZ3gDVQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits &> /tmp/tmp.tUERckA0hG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
Found non-empty wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits and wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
The reference image (wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits) and catalog (wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat) found
'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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 9251 out of 169655 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.833037
a=0.000000 b=1.000000 c=22.833037
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 115 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
2.0 pix Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
2.5 pix fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
2.6 pix fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.5 mag. Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
15.5 mag. Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
14.8 mag. fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
14.8 mag. fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.l9BVGj9JDp (6) ############
Parsing command line arguments...
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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits' -> 'wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=21275, passed=169635
Got 169635 stars (including 148116 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 169635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 974 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits -region wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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.ZKKiQC4Aqs (6) ############
Parsing command line arguments...
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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits' -> 'wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=21215, passed=170059
Got 170059 stars (including 148600 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat
util/solve_plate_with_UCAC5 got 170059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 974 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits -region wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.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.mVuxZ3gDVQ (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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=10118, passed=104964
Got 104964 stars (including 94706 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 104964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits -region wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.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.tUERckA0hG (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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=9776, passed=101915
Got 101915 stars (including 91991 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 101915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits -region wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits
Saving fully-calibrated image wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-31-52_20.00sec_-14.90C_LIGHT_0012.fits
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.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_2026-03-21_CI_Per-02-Q1b1x1_233341_TTUQ1b1x1_9974_6nJZhfur/wcs_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013.fits
Preparing the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out140067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out09666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194945.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: 2s
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Considering the candidate 194463_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194463_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:58:23.64 +45:31:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 1.306 244020770245938560 059.59887313182 +45.52844600622 14.7432 14.0334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194468_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194468_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:58:20.78 +44:22:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194471_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194471_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:03:54.70 +42:15:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.319 230704069526707712 060.97753831007 +42.25496908203 14.1386 13.4712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194472_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194472_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:30:30.62 +44:13:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.343 241562056088314880 052.62762332969 +44.23187253009 13.7645 12.9404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194474_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194474_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:54:57.28 +44:34:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.730 243827634156210432 058.73810676092 +44.57912933935 13.7455 12.8385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194480_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194480_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:19:30.15 +46:38:24.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)
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Considering the candidate 194482_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194482_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:06:51.83 +50:08:56.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 194487_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194487_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:59:24.76 +49:10:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 194488_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194488_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:14:55.85 +49:53:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 3.113 270599127384821632 063.73198397042 +49.88989454190 14.2754 13.5697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194489_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194489_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:58.94 +48:38:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194491_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194491_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:12:04.99 +45:52:31.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 194497_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194497_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:55:30.26 +44:16:25.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 194501_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194501_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:14:53.75 +41:34:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.562 239575960127804672 048.72409484023 +41.58289378381 13.6100 13.0924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194505_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194505_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:12:45.94 +42:32:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194508_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194508_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:36:39.26 +48:52:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194509_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194509_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:50:01.98 +45:38:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.881 244925354778235008 057.50796974550 +45.64201210612 13.4388 12.5663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194513_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194513_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:47.13 +41:53:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.654 336414003635578368 043.44612207122 +41.89819187573 13.5155 12.7916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194514_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194514_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:56:13.32 +42:31:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194518_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194518_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:01:04.27 +43:10:03.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 194519_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194519_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:15.25 +42:50:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.253 336604081707389312 043.31352637751 +42.84129238765 13.2442 12.5199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194520_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194520_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:29.10 +42:20:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.426 336529074398678656 043.37101646298 +42.33427311676 13.1720 12.7435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194521_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194521_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 194523_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194523_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:13:53.72 +43:50:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194540_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194540_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:09:13.95 +44:50:33.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 194547_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194547_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:36.48 +42:54:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194556_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194556_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:11.67 +40:52:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 3.298 336115207053011840 043.54762021339 +40.88278955100 12.0101 11.5257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194558_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194558_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:48.53 +40:58:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.237 336138537315356160 043.70225952150 +40.97855329028 11.8700 11.6874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194574_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194574_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:30:26.01 +48:06:27.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194589_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194589_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:17.32 +41:02:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.504 336163276326977280 043.57214111133 +41.03613853122 12.1486 11.7130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194592_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194592_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:51.02 +40:59:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.605 336138919569828096 043.71239739325 +40.98881485158 12.1279 11.4336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194593_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194593_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:03:48.34 +47:50:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194600_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194600_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:55.53 +40:49:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.284 336113218485614720 043.48090390315 +40.81820967913 12.2611 11.7830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194604_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194604_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:00.70 +44:52:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194606_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194606_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:03.07 +41:13:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.705 336192722622743552 043.51274852619 +41.22538770447 12.3540 11.9205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194607_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194607_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:43.32 +41:00:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.221 336138812193260672 043.68027396237 +41.01298755244 12.3636 12.0331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194612_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194612_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:57.04 +40:54:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.281 336161008584253312 043.48723177292 +40.91333109913 12.3107 11.6277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194616_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194616_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:18:46.43 +50:11:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194621_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194621_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:08:15.47 +41:27:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194627_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194627_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:47.15 +41:24:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.806 336207879564446464 043.44615999148 +41.40567403940 12.4589 11.7265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194638_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194638_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:57:48.56 +46:39:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.184 434375881168973568 044.45145987000 +46.65112091587 12.6281 11.7862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194646_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194646_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:33.29 +40:58:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.192 336139396308815232 043.63856801870 +40.98259141514 12.6466 12.2013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194661_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194661_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:22:06.41 +42:48:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194681_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194681_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:15.84 +40:59:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.834 336163177545127680 043.56572762547 +40.99774397488 12.9248 12.5414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194689_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194689_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:56:29.75 +44:55:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194712_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194712_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:22.33 +42:35:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194718_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194718_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:37:54.18 +42:35:59.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194723_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194723_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:32:06.91 +44:28:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194730_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194730_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:49.13 +41:10:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.590 336192177164043008 043.45474088670 +41.17643984032 12.8379 12.1609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194735_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194735_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:02:48.73 +47:05:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194741_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194741_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:28:48.91 +50:24:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194742_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194742_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:55.78 +41:06:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.745 336141805787805184 043.73220554864 +41.11634683380 13.0444 12.5561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194770_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194770_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:18:47.13 +47:00:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194778_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194778_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:51.82 +41:30:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.926 336211624775912576 043.46572143906 +41.51115597797 13.2039 12.7052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194782_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194782_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:30.64 +40:59:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.038 336139469325651712 043.62736673666 +40.98953946261 13.1791 12.5916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194785_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194785_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:54:04.48 +44:33:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194789_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194789_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:13:24.33 +49:46:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194793_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194793_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:17:28.95 +50:06:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194796_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194796_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:54:56.67 +48:35:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194809_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194809_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:43.96 +41:14:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.081 336204306151680128 043.43305569260 +41.23581622822 13.2969 12.7848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194811_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194811_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:39.21 +47:18:57.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194812_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194812_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:24:54.98 +41:57:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194818_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194818_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:56.42 +41:13:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.534 336192417682203008 043.48501988945 +41.23217333844 13.2540 12.5184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194819_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194819_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:40.08 +40:54:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.530 336114833393268608 043.66651216774 +40.91043385789 13.1369 12.6952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194831_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194831_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:04:29.20 +50:03:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194833_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194833_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:28:27.99 +50:27:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194838_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194838_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:55:25.54 +40:56:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.839 336136170790762624 043.85616889144 +40.94125309765 13.4135 12.8200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194853_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194853_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:11.87 +40:50:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.231 336112943607695232 043.54918931936 +40.84138582808 13.2709 12.5897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194855_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194855_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:40:04.19 +48:56:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194857_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194857_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:05:01.94 +46:19:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194859_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194859_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:55:15.20 +40:56:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.514 336134968199921024 043.81322720916 +40.94984034886 13.2923 12.8129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194865_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194865_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:50.48 +44:10:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194872_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194872_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:03:51.38 +41:13:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194874_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194874_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:18:41.81 +46:26:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194880_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194880_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:42.79 +40:53:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.345 336111878455774336 043.67812282248 +40.89560124461 13.1226 12.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194883_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194883_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:40:56.56 +41:16:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194894_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194894_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:47.38 +40:54:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.633 336135277437595008 043.69731253483 +40.90821266855 13.3501 12.6994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194895_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194895_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:57.45 +46:57:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194898_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194898_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:33:24.03 +47:54:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194899_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194899_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:39.59 +48:17:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194904_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194904_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:06:08.73 +47:46:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194909_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194909_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:04.65 +41:01:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.210 336164173977530752 043.51924327905 +41.03162656595 13.4062 12.8469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194911_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194911_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:31.90 +41:38:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.968 336401045716475776 043.38241416019 +41.64959175915 13.4160 12.8341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194912_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194912_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:15:48.87 +43:35:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194920_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194920_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:27.03 +40:54:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.285 336114936472492160 043.61302335413 +40.90488632570 13.5672 13.1805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194924_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194924_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:23:37.35 +49:57:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194935_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194935_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:36:42.10 +47:14:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194945_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 194945_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
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Considering the candidate 194947_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194947_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 194955_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194955_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:09:20.09 +46:50:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194958_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194958_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:45.69 +44:04:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 3.278 243705687144799744 056.18961720622 +44.08328559045 12.6897 10.8810 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194971_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194971_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:42.66 +41:22:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.935 336206367735962496 043.42723174286 +41.37692671761 13.5791 13.1008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194973_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194973_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:06:48.20 +41:50:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194975_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194975_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:29:03.29 +49:49:51.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194983_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194983_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:31.62 +47:51:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194985_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194985_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:35:03.70 +45:25:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194992_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 194992_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:29:42.27 +47:58:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195014_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 195014_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:22:50.04 +48:47:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195124_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 195124_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:38.84 +41:33:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180348_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 180348_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:00:26.67 +41:32:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180917_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 180917_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:58:30.69 +41:22:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24542_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 24542_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 04:14:56.23 +48:49:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141641_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 141641_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:36:21.43 +43:38:16.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 58753_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 58753_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:26:29.89 +47:31:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140067_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 140067_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:35.08 +43:26:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.522 432721086104969600 043.64558919455 +43.43572045864 13.0917 12.6274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35882_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 35882_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:23.22 +48:39:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126037_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 126037_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:59:56.40 +42:37:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152437_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 152437_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
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Considering the candidate 164433_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 164433_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 02:57:19.89 +41:48:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161035_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 161035_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:11:40.91 +41:38:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12752_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 12752_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:42:34.73 +50:15:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158186_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 158186_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 03:32:32.26 +41:26:30.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 134584_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 134584_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
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Considering the candidate 129714_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013
The candidate 129714_fd_Per-02-Q1b1x1_2026-03-21_23-32-59_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks