This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo
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
V Cnc,2461118.8257,9.48,0.05,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
V Cnc 20260319.3257 9.48CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:43.49 +17:17:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_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
U Cnc,2461118.8257,9.28,0.05,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
U Cnc 20260319.3257 9.28CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:46.47 +18:53:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.89 08:23:00.29 +17:45:45.7
206.26196 27.95662 galactic Cnc Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:23:00.29 +17:45:45.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8257,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3257 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:00.29 +17:45:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.53 08:23:41.11 +18:46:29.3
205.26126 28.47906 galactic Cnc Second-epoch detections are separated by 4.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 662449918876959872 | 08:23:39.57 +18:45:48.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 662449918876959872,2461118.8257,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 662449918876959872 20260319.3257 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:41.11 +18:46:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.52 08:23:13.02 +18:34:49.1
205.42122 28.30492 galactic Cnc Second-epoch detections are separated by 2.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:23:13.02 +18:34:49.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8257,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3257 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:13.02 +18:34:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.56 08:24:56.39 +18:57:21.0
205.19158 28.82130 galactic Cnc Second-epoch detections are separated by 2.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:24:56.39 +18:57:21.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8257,13.56,0.05,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 20260319.3257 13.56CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:56.39 +18:57:21.0 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 662542514075320832,2461118.8257,12.85,0.05,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 662542514075320832 20260319.3257 12.85CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:43.61 +18:51:38.5 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_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
VARIABLE_NAME,2461118.8257,12.95,0.05,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
VARIABLE_NAME 20260319.3257 12.95CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:38:24.41 +16:01:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_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
VARIABLE_NAME,2461118.8257,14.12,0.05,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
VARIABLE_NAME 20260319.3257 14.12CV 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:06.28 +15:01:38.5 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91374440 23.12.2025 09:55:37.516 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
First image: 2461032.91374440 23.12.2025 09:55:37.516 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Last image: 2461118.82596008 19.03.2026 07:49:12.951 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11688
Objects passed selection criteria: 11680
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 10995.2
Average stars matched: 10835.2 (98.5448 %)
Memory usage VmPeak: 117212 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:56:05 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91374440 23.12.2025 09:55:37.516 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
First image: 2461032.91374440 23.12.2025 09:55:37.516 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Last image: 2461118.82596008 19.03.2026 07:49:12.951 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 17 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): 61759
Objects passed selection criteria: 61646
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 57099
Average stars matched: 55606 (97.3852 %)
Memory usage VmPeak: 160956 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:57:04 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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: 2461118.82538079
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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits'
wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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 08:53:20.045 +13:59:34.17
Second-epoch image center 08:53:28.160 +14:00:14.96
Angular distance between the image centers 0.03 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 08:53:20.045 +13:59:34.17
Second-epoch image center 08:53:30.703 +14:00:21.90
Angular distance between the image centers 0.05 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 08:53:28.160 +14:00:14.96
Second-epoch second image center 08:53:30.703 +14:00:21.90
Angular distance between the image centers 0.01046 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits &> /tmp/tmp.lnvuZoZ9Ru
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits &> /tmp/tmp.rkM3Ior9qJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits &> /tmp/tmp.fBoVUCtRvg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.KIEEZpdSGg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits) and catalog (wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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 6025 out of 12162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.970611
a=0.000000 b=1.000000 c=22.970611
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
2.2 pix Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
2.5 pix fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
2.5 pix fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
15.4 mag. Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
15.4 mag. Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
15.0 mag. fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
15.0 mag. fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lnvuZoZ9Ru (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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits' -> 'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=842, passed=12162
Got 12162 stars (including 11304 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
util/solve_plate_with_UCAC5 got 12162 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 964 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits -region wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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.rkM3Ior9qJ (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/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits' -> 'wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=866, passed=12142
Got 12142 stars (including 11261 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat
util/solve_plate_with_UCAC5 got 12142 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 962 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits -region wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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.fBoVUCtRvg (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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=572, passed=9975
Got 9975 stars (including 9396 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 9975 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 954 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 954 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: 0.51"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.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.KIEEZpdSGg (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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=546, passed=9972
Got 9972 stars (including 9422 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 9972 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 955 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits'
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits'
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out00399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01986.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20577_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20577_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:52:54.35 +14:47:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.173 608947713131692416 133.22643840389 +14.79876167146 12.1324 11.7078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20580_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20580_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 09:17:43.91 +09:57:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.479 590972725242144768 139.43260656440 +09.95619282861 12.1934 11.6531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20581_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20581_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:32:11.57 +16:04:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.015 658666774243171584 128.04849701247 +16.08222749509 12.4014 11.9800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20584_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20584_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:58:45.42 +15:03:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.297 610315784770223360 134.68917591694 +15.05262422362 12.5113 12.0239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20586_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20586_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:51:27.35 +11:53:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.989 604921512005265664 132.86420661302 +11.89070531726 12.6189 12.1625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20590_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 20590_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:52:47.93 +16:12:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.591 611439485654581888 133.19975705510 +16.20734267995 12.4111 11.9600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01986_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 01986_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00399_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 00399_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cnc-05-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 ####
08:35:46.47 +18:53:42.8
08:21:43.49 +17:17:03.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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 08:53:20.045 +13:59:34.17
Second-epoch image center 08:53:28.160 +14:00:14.96
Angular distance between the image centers 0.03 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 08:53:20.045 +13:59:34.17
Second-epoch image center 08:53:30.703 +14:00:21.90
Angular distance between the image centers 0.05 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 08:53:28.160 +14:00:14.96
Second-epoch second image center 08:53:30.703 +14:00:21.90
Angular distance between the image centers 0.01046 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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits &> /tmp/tmp.Y6z09xZBEo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits &> /tmp/tmp.Q1WRh6RsLp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits &> /tmp/tmp.OSEsr3joGl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.8neFOvoLlY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits and wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits) and catalog (wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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 6038 out of 65227 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.878237
a=0.000000 b=1.000000 c=22.878237
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
2.1 pix Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
2.4 pix fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
2.4 pix fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
15.5 mag. Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
15.5 mag. Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
15.1 mag. fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
15.1 mag. fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Y6z09xZBEo (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/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits' -> 'wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=3854, passed=65210
Got 65210 stars (including 61255 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat
util/solve_plate_with_UCAC5 got 65210 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 963 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits -region wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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.Q1WRh6RsLp (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/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits' -> 'wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3851, passed=65442
Got 65442 stars (including 61478 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat
util/solve_plate_with_UCAC5 got 65442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 960 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits -region wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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.OSEsr3joGl (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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2714, passed=50141
Got 50141 stars (including 47353 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 50141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 950 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.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.8neFOvoLlY (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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2687, passed=49172
Got 49172 stars (including 46429 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 49172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 952 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_Cnc-05-Q2b1x1_2025-12-23_03-56-52_20.00sec_-15.00C_LIGHT_0523.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.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_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out79731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out79759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80121.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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 79731_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79731_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 09:12:19.00 +11:13:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.916 592122406383453696 138.07934140730 +11.22743824250 14.3867 13.8406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79739_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79739_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:22:54.10 +09:40:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.927 600332013032479744 125.72488590647 +09.66994207247 13.6281 13.2140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79742_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79742_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:37:31.31 +09:51:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.188 601239007045961984 129.38031274425 +09.86210270747 14.1216 13.5630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79747_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79747_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:49:15.88 +09:28:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.369 597285124576926720 132.31606838263 +09.48256134312 13.9627 13.5052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79753_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79753_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:23:38.61 +17:44:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 4.503 662314129191205504 125.91216760153 +17.73727594608 13.1836 12.5403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79757_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79757_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:21:56.79 +12:17:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.883 649327419397237120 125.48658837996 +12.29710507310 13.4195 12.7855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79759_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79759_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79762_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79762_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:45:20.17 +13:16:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.954 608353328313916672 131.33396176788 +13.28050322531 13.9801 13.5250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79763_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79763_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:25:21.29 +18:19:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.129 662374941630400384 126.34011589283 +18.33197757763 13.2710 12.7260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79765_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79765_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:22:06.63 +18:20:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 4.431 662409271306516096 125.52668762829 +18.33921166418 13.1453 12.5159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79766_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79766_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:23:07.67 +10:12:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.188 600573939950876544 125.78298750554 +10.20171101168 13.5320 13.0154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79767_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79767_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 79772_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79772_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:22:49.34 +17:33:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.481 656306466376313984 125.70659707862 +17.56636391821 13.2186 12.7931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79775_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79775_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79783_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79783_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79785_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79785_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79792_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79792_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:23:00.38 +18:34:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.898 662437996047766784 125.75295773220 +18.57372586877 12.4382 11.7164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79794_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79794_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:23:44.34 +18:38:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.123 662445069857490688 125.93622543316 +18.63642841369 12.3213 11.8130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79798_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79798_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:22:07.86 +16:44:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.226 656048837058004352 125.53425870125 +16.74280954059 11.9018 11.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79799_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79799_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79805_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79805_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:36:06.76 +10:20:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.040 601329476236898176 129.02834053869 +10.34517739907 11.1127 10.8120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79829_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79829_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:44:30.51 +15:55:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.341 610060040941874816 131.12721101856 +15.91729609341 11.6466 11.2048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79886_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 79886_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 79961_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79961_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:29:47.54 +15:32:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.082 652617295626962304 127.44748420203 +15.54826970576 13.4029 12.9306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79970_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79970_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:38:33.41 +15:30:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.395 657741157250540160 129.63914316753 +15.51027100946 13.6636 13.2022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79987_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79987_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:28:08.20 +11:41:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.341 602660538142123264 127.03568174326 +11.69468004026 13.8677 13.3197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79998_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 79998_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:27:58.40 +11:43:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 80054_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80054_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:42:55.50 +14:05:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.658 609225515912709376 130.73130626639 +14.09795940221 14.1663 13.6863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80058_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80058_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:43:17.46 +16:54:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.783 658228103462606336 130.82260931595 +16.91175440354 14.1258 13.6170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80062_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80062_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:48:14.09 +11:33:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.244 598949171001193344 132.05864592233 +11.55877896776 13.8049 13.1838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80068_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80068_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:36:13.27 +15:18:01.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 80073_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80073_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:31:36.47 +15:25:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.600 651882443901975808 127.90185864913 +15.42821954166 14.0605 13.6017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80079_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80079_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 09:01:31.19 +15:10:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.111 610300185449029632 135.38001802408 +15.17403010445 14.0770 13.6674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80095_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80095_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:52:30.04 +18:02:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.565 659958906564013056 133.12562287357 +18.04688999317 14.2981 13.8237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
Preparing report for the candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
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Considering the candidate 80129_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80129_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 09:15:16.70 +09:45:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.300 590882913181519616 138.81994808510 +09.75311663751 14.1252 13.6209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80131_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80131_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:57:41.46 +16:32:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.261 611514355524292352 134.42238749814 +16.54593308320 14.2495 13.7115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80165_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80165_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:38:17.07 +12:26:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 3.334 602936584280068864 129.57051862152 +12.44221201915 14.0710 13.0585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80183_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 80183_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:35:04.18 +15:29:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.875 657835612171827968 128.76723355850 +15.49386161398 14.4079 13.9224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10275_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 10275_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks
**** FOUND 08:21:43.48 +17:17:03.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 01730_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049
The candidate 01730_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049 did not pass the final checks