This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J232722.82+701742.6,2461129.9563,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J232722.82+701742.6 20260330.4563 12.99CV 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:27:22.67 +70:17:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.4563 2461129.9563 12.68 00:41:42.73 +65:51:13.6
121.93618 3.00083 galactic Cas Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527630341405576192 | 00:41:44.80 +65:51:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.4563* 00 41 42.73 +65 51 13.6 12.7 U Cas 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
Gaia DR3 527630341405576192,2461129.9563,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527630341405576192 20260330.4563 12.68CV 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:42.73 +65:51:13.6 ;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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.9563,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.4563 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:52:04.97 +72:46:07.0 ;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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_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 30.4563* 00 35 14.15 +70 44 49.5 11.6 U Cas 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
NSVS J0035140+704447,2461129.9563,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0035140+704447 20260330.4563 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:14.15 +70:44:49.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_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 30.4563* 01 04 32.99 +71 02 19.4 11.9 U Cas 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
AD Cas,2461129.9563,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AD Cas 20260330.4563 11.90CV 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:04:32.99 +71:02:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1301,2461129.9563,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1301 20260330.4563 13.15CV 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:03.93 +67:50:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20_00sec_-10_00C_LIGHT_0398_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20_00sec_-10_00C_LIGHT_0397_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461129.95768517 30.03.2026 10:58:53.999 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
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: 3 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): 14594
Objects passed selection criteria: 14520
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 10400
Average stars matched: 9787.5 (94.1106 %)
Memory usage VmPeak: 119384 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 Mon Mar 30 06:02:01 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
First image: 2461036.59057495 27.12.2025 02:10:15.676 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Last image: 2461129.95768517 30.03.2026 10:58:53.999 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 101
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 25 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): 96848
Objects passed selection criteria: 96670
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 73415.5
Average stars matched: 68351.5 (93.1023 %)
Memory usage VmPeak: 2452108 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 Mon Mar 30 06:08:41 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461129.95495141
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits'
wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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 00:00:02.007 +69:59:50.87
Second-epoch image center 00:00:37.755 +69:59:17.71
Angular distance between the image centers 0.05 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 00:00:02.007 +69:59:50.87
Second-epoch image center 00:00:42.877 +69:59:34.02
Angular distance between the image centers 0.06 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 00:00:37.755 +69:59:17.71
Second-epoch second image center 00:00:42.877 +69:59:34.02
Angular distance between the image centers 0.00859 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.lgkCr6IKjd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.9IAlyIZ66g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits &> /tmp/tmp.oUB3ckgW17
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits &> /tmp/tmp.tqBBZhV2jd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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 9568 out of 16658 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942221
a=0.000000 b=1.000000 c=22.942221
From vast_summary.log: estimated ref. image limiting mag.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.5 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.7 pix fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
2.5 pix fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Limiting magnitude estimates:
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.0 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
14.0 mag. fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
14.1 mag. fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.lgkCr6IKjd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1610, passed=16658
Got 16658 stars (including 15034 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 16658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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.9IAlyIZ66g (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1667, passed=16773
Got 16773 stars (including 15086 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 16773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 339 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.96"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 7.12"
Estimated accuracy of the plate solution: 5.50"
Excluding outliers - 385 stars left (next iteration limit 310)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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.oUB3ckgW17 (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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=468, passed=7891
Got 7891 stars (including 7414 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat
util/solve_plate_with_UCAC5 got 7891 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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: 0.68"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.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.tqBBZhV2jd (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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, passed=8186
Got 8186 stars (including 7689 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 8186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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: 0.58"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits'
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21761.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21426_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 21426_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:13:10.34 +73:51:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21761_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 21761_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:58:18.30 +70:30:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 1.755 533092719470319232 014.57753939756 +70.50725673866 10.3056 9.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits exists and is non-empty
wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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 00:00:02.007 +69:59:50.87
Second-epoch image center 00:00:37.755 +69:59:17.71
Angular distance between the image centers 0.05 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 00:00:02.007 +69:59:50.87
Second-epoch image center 00:00:42.877 +69:59:34.02
Angular distance between the image centers 0.06 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 00:00:37.755 +69:59:17.71
Second-epoch second image center 00:00:42.877 +69:59:34.02
Angular distance between the image centers 0.00859 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/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits &> /tmp/tmp.J0Zm2pDmoJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.WmdH9PYyfC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits &> /tmp/tmp.3bw3F9vfVh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits &> /tmp/tmp.q8fj2JfFsT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits and wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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 9832 out of 114234 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779293
a=0.000000 b=1.000000 c=22.779293
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 83 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
2.3 pix Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
2.5 pix fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
2.4 pix fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Limiting magnitude estimates:
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
15.2 mag. Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
14.2 mag. fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
14.3 mag. fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.J0Zm2pDmoJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=12405, passed=114192
Got 114192 stars (including 101585 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 114192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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.WmdH9PYyfC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=12319, passed=113226
Got 113226 stars (including 100709 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 113226 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.8'
Seting catalog search parameters based on the expected field of view 932.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012956 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010364 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 349 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.18"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.75"
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 414 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.74"
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 384 stars left (next iteration limit 322)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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.3bw3F9vfVh (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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3126, passed=51836
Got 51836 stars (including 48648 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat
util/solve_plate_with_UCAC5 got 51836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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: 0.64"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 970 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.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.q8fj2JfFsT (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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3240, passed=58457
Got 58457 stars (including 55141 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 58457 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-54-57_20.00sec_-10.00C_LIGHT_0397.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.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_2026-03-30_CI_Cep-03-Q2b1x1_055929_TTUQ2b1x1_1870_oDkQaHnI/wcs_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398.fits
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out133081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out140072.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out137205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87145.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 133081_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133081_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:22:59.53 +70:45:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.047 2227203154456356096 350.74935018682 +70.75412038227 13.9350 13.3068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133088_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133088_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:16:06.29 +73:17:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133090_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133090_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:40:31.65 +70:27:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.750 2215332556345603584 355.13332642352 +70.46511035795 12.7795 11.6027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133095_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133095_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:16:44.06 +66:55:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.721 2213544368181094016 349.18475214617 +66.92294696455 13.3195 12.5902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133096_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133096_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:56:55.47 +73:29:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.509 538344158801892224 014.23093368117 +73.49159159226 12.8316 12.3158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133098_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133098_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 133101_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133101_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 22:55:25.03 +70:54:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.317 2226692298166099328 343.85529876740 +70.91552040842 12.7169 12.3846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133102_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133102_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:34:14.28 +66:41:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.525 527728133518153984 008.55984867052 +66.69906717669 11.6763 11.0848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 133103_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 133103_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:11:30.79 +67:30:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134106_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 134106_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:58:18.21 +70:30:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.203 533092719470319232 014.57753939756 +70.50725673866 10.3056 9.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134471_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 134471_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:54:13.66 +65:47:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 0.854 2017558623853435008 358.55734188211 +65.79435521954 11.2338 10.5712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134758_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 134758_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:42:31.16 +71:22:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 0.318 536387955818667136 010.63010396732 +71.37979557420 11.4282 10.8984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135218_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 135218_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:07:05.83 +72:45:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.567 537453245145728640 001.77455519707 +72.76222424347 11.7777 10.9369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 135795_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 135795_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:48:12.82 +67:47:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136257_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 136257_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:18:16.50 +68:07:15.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136648_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 136648_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 01:18:27.87 +72:54:01.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 136721_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 136721_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:21:26.68 +67:49:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.226 528793727785360768 005.36089946286 +67.82128590842 12.1777 11.4156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 136907_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 136907_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:04:07.65 +70:48:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.397 2225902814458637440 346.03123343782 +70.80750764371 12.5418 10.4904 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137056_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137056_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:49:34.61 +70:27:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.500 536088029663084672 012.39216278569 +70.45847960187 12.0787 11.1811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137175_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137175_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:25:32.41 +71:49:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.189 537107002062677504 006.38520014676 +71.82039884427 12.2584 11.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137205_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
Preparing report for the candidate 137205_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
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Considering the candidate 137279_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137279_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:05:14.39 +67:48:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.110 528971028333420032 001.31072819353 +67.81295250029 12.0413 10.9764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137314_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137314_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:01:39.92 +73:38:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137477_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137477_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:27:18.98 +65:35:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.809 2209433401588564096 351.82965697799 +65.59600128527 12.8166 12.2376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137544_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137544_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:07:10.86 +67:17:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.575 528529363957640960 001.79638214352 +67.28539985081 12.5040 11.8785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137554_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137554_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:36:41.24 +67:50:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.430 2211075174304617472 354.17287633086 +67.83941788104 12.7199 12.1802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137591_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137591_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 22:52:34.48 +67:58:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.163 2213323782961042048 343.14370035397 +67.97034545165 12.9279 12.2434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137674_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
Preparing report for the candidate 137674_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
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Considering the candidate 137972_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137972_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 01:18:59.54 +72:52:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137984_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 137984_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 01:16:29.80 +71:43:18.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 138020_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138020_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:11:48.44 +66:20:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.000 528186870384605568 002.95170465070 +66.34883586507 11.3427 9.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138107_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138107_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:37:57.99 +72:54:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138130_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138130_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 22:57:25.18 +65:18:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.471 2211850677897534720 344.35695511665 +65.31164701886 13.1421 12.5022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138230_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138230_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:27:09.19 +65:38:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.707 2209437417376458752 351.78873895239 +65.64309927755 12.3473 11.2063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138328_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138328_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:37:18.54 +68:45:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.105 2214177175782308096 354.32806564087 +68.75130453177 12.8075 12.1881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138471_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138471_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:01:01.15 +70:56:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.471 531238186950121344 000.25587907012 +70.94470229758 12.7310 12.1257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138527_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138527_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:39:31.11 +70:47:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.595 2215543422059999360 354.88008477910 +70.78645538775 12.8998 12.0800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138735_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138735_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:39:03.93 +74:02:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138770_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138770_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:57:25.92 +72:50:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.743 2227866301706866944 359.35904823296 +72.84079396743 13.1316 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138788_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138788_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:58:16.58 +67:41:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.371 526676618144395008 014.57001647800 +67.68980431439 12.5203 11.8122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138796_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138796_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:44:08.63 +70:18:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.159 2215271636530512896 356.03769934709 +70.30415224222 13.1224 12.5828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138870_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 138870_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:33:47.84 +68:01:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.800 2213722424645211776 353.44823707432 +68.03291102348 12.6517 11.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139161_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139161_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:04:05.69 +65:12:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139164_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139164_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:33:05.40 +71:00:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139363_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139363_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 01:15:39.17 +71:34:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139507_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139507_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:53:53.42 +71:28:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.628 2215671515164455808 358.47312796188 +71.47339441053 13.3158 12.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139609_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139609_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:38:43.34 +71:10:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.754 536357130833491328 009.68207779436 +71.17118027080 12.8048 12.2871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139652_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139652_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:53:42.98 +71:28:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.444 2215671205926806400 358.42880542986 +71.47485861729 13.4392 12.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139696_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139696_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:56:41.66 +68:28:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.523 526811965455678976 014.17568528086 +68.48388077194 12.4976 11.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139903_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139903_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:28:56.37 +72:14:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.030 2227590977123340928 352.23645953366 +72.24962439583 13.1755 12.5190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139989_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 139989_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:03:51.43 +71:11:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.379 2228177905874191616 345.96631394966 +71.19660839083 11.5235 9.9396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140072_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140072_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:15:50.66 +72:17:55.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 140099_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
Preparing report for the candidate 140099_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
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Considering the candidate 140165_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140165_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 140181_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140181_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:17:24.73 +66:30:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.994 2210515286667075200 349.35392903126 +66.51245397979 13.5025 12.7794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140375_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140375_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:23:34.26 +65:45:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.638 2210201307379041280 350.89302807534 +65.76007922392 13.4497 12.7099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140400_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140400_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:59:03.96 +66:50:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.733 2209837369029096960 359.76823712879 +66.83394184161 12.6460 11.4400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140582_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140582_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:06:23.71 +70:05:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.666 530802505467851136 001.59983489373 +70.09357433179 12.3990 11.2053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140628_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140628_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:34:47.23 +72:45:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140693_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140693_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:12:44.10 +67:24:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140764_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140764_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:02:14.34 +67:23:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.232 528569156833235840 000.56050824932 +67.38804026472 12.9547 12.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140852_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140852_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:28:05.20 +68:56:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.988 529718898099046400 007.02314929018 +68.93397850069 12.4933 11.1939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140863_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140863_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:15:06.34 +72:07:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.574 537185514064300544 003.77688980955 +72.12785690378 13.1223 12.2165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140915_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140915_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:17:31.45 +71:02:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.783 2227364031052526464 349.38597678284 +71.04015230681 13.4228 12.4311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140976_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 140976_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:14:27.48 +70:35:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.116 2227160071644748672 348.61536856477 +70.58435941554 13.1961 11.2902 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141365_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141365_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:34:58.63 +71:19:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.535 2227614547902974720 353.74553732794 +71.31815540316 13.6913 12.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141409_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141409_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:28:13.74 +72:50:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.820 2228418119105210496 352.05872549595 +72.84021521563 13.1313 11.9791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141442_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141442_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:22:15.58 +71:28:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.967 537086729817217920 005.56620568228 +71.47902706549 12.3301 11.0874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141500_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141500_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:02:11.79 +72:23:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.068 537427303543071616 000.55277375145 +72.38571198829 13.6560 13.0435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141724_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141724_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:38:26.22 +70:36:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.550 2215505415890663936 354.60973141621 +70.60987797252 13.6718 12.8736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141787_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141787_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:20:01.03 +65:32:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.088 2210173853947667456 350.00379424312 +65.53556901582 13.8187 11.8942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141951_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141951_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:11:50.20 +71:05:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.507 2227422717485168896 347.95898077844 +71.09484499278 13.9737 13.3356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141992_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 141992_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:22:29.91 +73:14:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142083_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 142083_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:41:53.32 +70:04:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.629 2215251295564747008 355.47507453400 +70.07148932430 13.8547 12.9654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142388_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 142388_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:50:42.48 +71:46:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.944 2215728071293581568 357.67772279537 +71.76743841346 13.8725 13.1718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142845_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 142845_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 23:24:43.34 +69:57:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.511 2215098669605650560 351.17872789775 +69.95157462613 13.7193 13.2424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13668_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 13668_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:13:10.27 +73:51:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30532_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 30532_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:10:08.81 +72:28:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45630_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
Preparing report for the candidate 45630_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
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Considering the candidate 31670_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
Preparing report for the candidate 31670_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
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Considering the candidate 66618_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 66618_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks
**** FOUND 00:45:36.06 +68:37:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.505 529790469437403776 011.40143338349 +68.62329590309 11.9792 10.5210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125482_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398
The candidate 125482_fd_Cep-03-Q2b1x1_2026-03-30_05-58-53_20.00sec_-10.00C_LIGHT_0398 did not pass the final checks