This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2
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
VARIABLE_NAME,2461118.8201,10.02,0.05,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 20260319.3201 10.02CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:01:55.69 +21:34:12.5 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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
V Cnc,2461118.8201,9.71,0.05,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 20260319.3201 9.71CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:42.78 +17:17:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 14.10 07:46:26.44 +26:36:50.0
193.76873 23.16643 galactic Gem Second-epoch detections are separated by 3.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:46:26.44 +26:36:50.0 (user input) | T | P | (position from user input) SpType: G2 (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,2461118.8201,14.10,0.05,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 20260319.3201 14.10CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:26.44 +26:36:50.0 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.98 07:51:14.48 +19:30:42.5
201.36569 21.63680 galactic Gem Second-epoch detections are separated by 1.8" and 3.3 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 | 07:51:14.48 +19:30:42.5 (user input) | T | P | (position from user input) SpType: F9 (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,2461118.8201,13.98,0.05,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 20260319.3201 13.98CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:14.48 +19:30:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 14.06 07:46:33.53 +24:50:55.4
195.57621 22.58060 galactic Gem Second-epoch detections are separated by 2.0" and 3.4 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 | 07:46:33.53 +24:50:55.4 (user input) | T | P | (position from user input) SpType: G4 (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,2461118.8201,14.06,0.05,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 20260319.3201 14.06CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:33.53 +24:50:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,13.88,0.05,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 20260319.3201 13.88CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:50.85 +26:38:28.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.62 07:45:57.50 +25:58:21.8
194.38285 22.84510 galactic Gem Second-epoch detections are separated by 2.8" and 3.7 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 | 07:45:57.50 +25:58:21.8 (user input) | T | P | (position from user input) SpType: F9 (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,2461118.8201,13.62,0.05,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 20260319.3201 13.62CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:57.50 +25:58:21.8 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.50 08:33:34.76 +18:17:13.7
206.76138 30.48734 galactic Cnc Second-epoch detections are separated by 7.2" and 3.4 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 659593353307603200 | 08:33:35.37 +18:17:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 659593353307603200,2461118.8201,13.50,0.05,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 659593353307603200 20260319.3201 13.50CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:34.76 +18:17:13.7 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.63 07:46:14.11 +26:44:59.3
193.61272 23.16947 galactic Gem Second-epoch detections are separated by 0.7" and 3.3 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 | Gaia DR3 874912085468209664 | 07:46:13.46 +26:45:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (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
Gaia DR3 874912085468209664,2461118.8201,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 874912085468209664 20260319.3201 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:14.11 +26:44:59.3 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.15 07:45:12.65 +26:14:13.2
194.05096 22.77870 galactic Gem Second-epoch detections are separated by 4.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 868889304368489472 | 07:45:12.11 +26:14:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 868889304368489472,2461118.8201,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 868889304368489472 20260319.3201 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:12.65 +26:14:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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,2461118.8201,12.94,0.05,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 20260319.3201 12.94CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:48:42.68 +21:26:22.0 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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,2461118.8201,13.20,0.05,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 20260319.3201 13.20CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:01.69 +23:28:58.7 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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,2461118.8201,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3201 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:13.59 +19:34:59.9 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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,2461118.8201,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3201 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:57.83 +17:27:51.9 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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,2461118.8201,14.31,0.05,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 20260319.3201 14.31CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:43:17.53 +19:56:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0829149+182314,2461118.8201,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0829149+182314 20260319.3201 12.93CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:15.11 +18:23:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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
SX Cnc,2461118.8201,12.88,0.05,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
SX Cnc 20260319.3201 12.88CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:51:19.65 +25:33:24.7 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 12.59 08:52:33.10 +26:10:11.7
199.42493 37.14536 galactic Cnc Second-epoch detections are separated by 0.6" and 3.7 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 | 08:52:33.10 +26:10:11.7 (user input) | T | P | (position from user input) SpType: G3 (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,2461118.8201,12.59,0.05,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 20260319.3201 12.59CV 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:52:33.10 +26:10:11.7 ;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-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_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: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
First image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Last image: 2461118.82033228 19.03.2026 07:41:06.709 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13908
Objects passed selection criteria: 13891
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: 13093.2
Average stars matched: 12874.2 (98.3274 %)
Memory usage VmPeak: 119224 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 02:58:34 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: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
First image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Last image: 2461118.82033228 19.03.2026 07:41:06.709 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 277
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 28 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): 79176
Objects passed selection criteria: 79021
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 72304.8
Average stars matched: 70474.2 (97.4684 %)
Memory usage VmPeak: 1935688 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 02:59:55 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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: 2461118.81979455
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:39.623 +22:01:19.45
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:38.255 +22:01:11.09
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:18:39.623 +22:01:19.45
Second-epoch second image center 08:18:38.255 +22:01:11.09
Angular distance between the image centers 0.00577 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits &> /tmp/tmp.6Y4bjGTfyI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits &> /tmp/tmp.fylUcraRuQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits &> /tmp/tmp.WXXs8acmtK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.SPoeu6EGwg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
Found non-empty wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
The reference image (wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits) and catalog (wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat) found
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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 7184 out of 14630 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.976505
a=0.000000 b=1.000000 c=22.976505
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
2.1 pix Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
2.5 pix fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
2.5 pix fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Limiting magnitude estimates:
15.5 mag. Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
15.5 mag. Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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.6Y4bjGTfyI (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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1109, passed=14630
Got 14630 stars (including 13511 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
util/solve_plate_with_UCAC5 got 14630 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 975 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits -region wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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.fylUcraRuQ (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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1116, passed=14643
Got 14643 stars (including 13509 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
util/solve_plate_with_UCAC5 got 14643 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 975 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits -region wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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.WXXs8acmtK (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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=723, passed=11715
Got 11715 stars (including 10983 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 11715 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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.SPoeu6EGwg (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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=716, passed=11705
Got 11705 stars (including 10978 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 11705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
Saving fully-calibrated image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits'
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out14415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20826.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20826_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 20826_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20846_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 20846_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14415_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 14415_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11161_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 11161_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:35:46.21 +18:53:45.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cnc-02-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 ####
08:21:42.78 +17:17:08.2
08:01:55.69 +21:34:12.5
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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits exists and is non-empty
wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:39.623 +22:01:19.45
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:38.255 +22:01:11.09
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:18:39.623 +22:01:19.45
Second-epoch second image center 08:18:38.255 +22:01:11.09
Angular distance between the image centers 0.00577 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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits &> /tmp/tmp.fS11yZb9OW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits &> /tmp/tmp.by8dHQfCp8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits &> /tmp/tmp.HuFaARm9dH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.IR3RvaIKEV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
Found non-empty wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
The reference image (wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits) and catalog (wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat) found
'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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 7219 out of 84420 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.884013
a=0.000000 b=1.000000 c=22.884013
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 169 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
2.0 pix Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
2.4 pix fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
2.4 pix fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Limiting magnitude estimates:
15.6 mag. Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
15.6 mag. Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
15.1 mag. fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
15.1 mag. fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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.fS11yZb9OW (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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=5639, passed=84389
Got 84389 stars (including 78614 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
util/solve_plate_with_UCAC5 got 84389 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 976 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits -region wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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.by8dHQfCp8 (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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=5720, passed=84301
Got 84301 stars (including 78450 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
util/solve_plate_with_UCAC5 got 84301 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits -region wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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.HuFaARm9dH (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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3826, passed=61350
Got 61350 stars (including 57463 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 61350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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.IR3RvaIKEV (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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3816, passed=61065
Got 61065 stars (including 57185 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 61065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Saving fully-calibrated image wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.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-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out04842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out44370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68829.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
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: 9s
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Considering the candidate 100509_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100509_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100510_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100510_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:16:35.76 +17:19:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.248 656998334069186688 124.14848223139 +17.31824247331 14.4641 13.9429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100511_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100511_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:17:08.86 +20:57:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.943 675804277870112256 124.28701418769 +20.95677336077 14.4704 13.8818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100515_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100515_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:48:14.64 +23:52:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.706 867548144997145472 117.06178754310 +23.87185393569 13.6791 13.1634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100526_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100526_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:47:44.08 +24:19:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.841 867624011299303424 116.93453241925 +24.31879198048 13.7984 13.3124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100531_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100531_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:21:13.48 +16:58:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.482 656070586772284032 125.30630384428 +16.96702692410 14.0063 13.6190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100532_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100532_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:49:13.02 +26:04:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.474 874090101744358016 117.30461841131 +26.07198090942 13.4768 12.7495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100536_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100536_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:48:38.01 +20:14:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.099 661573779907236992 132.15835745317 +20.23466610705 13.9971 13.4020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100537_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100537_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100538_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100538_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100541_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100541_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:45:56.47 +24:45:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.734 867851369688610304 116.48514255449 +24.75570812144 13.2718 12.6212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100543_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100543_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:50:07.16 +17:53:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.822 668517092758487040 117.52990873207 +17.88952878596 13.3025 12.7072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100545_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100545_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100546_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100546_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:50:01.81 +26:28:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.292 874115699749713536 117.50803638279 +26.47209820235 13.4322 12.7644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100554_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100554_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:38:25.02 +22:18:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.750 665981137908886016 129.60402520992 +22.30765212919 13.7030 13.0500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100560_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100560_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100569_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100569_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100572_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100572_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:48:03.29 +20:56:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.236 673672599701823872 117.01367309412 +20.94071306195 13.7710 13.2087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100573_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100573_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:30.66 +26:35:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.352 874906111169831168 116.62785926081 +26.59891316365 12.9925 12.5593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100574_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100574_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:49.60 +25:21:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.126 868034919410912512 116.70824079248 +25.36274024246 13.0868 12.6351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100584_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100584_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100585_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100585_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100589_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100589_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:09:27.57 +18:37:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.662 669374810610074112 122.36516247540 +18.61834953375 13.7896 13.1395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100590_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100590_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:45:07.61 +24:39:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.474 867844188503324416 116.28127005184 +24.66520593487 12.8098 12.1770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100591_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100591_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:45:24.42 +25:24:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.609 868026810512553856 116.35315369298 +25.40409974120 12.5815 11.8795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100592_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100592_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:22.63 +26:23:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 100593_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100593_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:47:24.49 +26:22:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 100594_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100594_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:47:25.83 +26:44:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.962 874885594109461248 116.85673930130 +26.73517056840 12.6419 11.9693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100595_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100595_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:45:59.58 +25:13:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.864 868008771650048384 116.49941178140 +25.21706016613 12.7062 12.2332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100596_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100596_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:48:05.07 +26:53:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.327 874894016541865600 117.02022611568 +26.89651522266 12.4875 11.8380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100597_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100597_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100602_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100602_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:48:45.82 +26:42:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.422 874876389996317568 117.19166813634 +26.70665176944 12.2701 11.6016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100607_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100607_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:45:38.13 +26:27:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.069 874898311509252480 116.40982016809 +26.45122921903 11.8060 11.1126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100608_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100608_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:17.69 +25:34:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.335 868053057055761152 116.57335461693 +25.57947756791 11.8761 11.2970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100610_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100610_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:33:35.45 +18:17:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.463 659593353307603200 128.39738846392 +18.28550795459 11.6817 10.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100613_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100613_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:01:55.69 +21:34:12.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 100626_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100626_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100632_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100632_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 100636_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100636_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100644_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100644_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 100647_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100647_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 100650_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100650_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100651_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100651_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100652_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100652_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100653_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100653_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100654_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100654_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100655_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100655_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100658_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100658_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100659_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100659_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100660_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100660_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 100663_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100663_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100666_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100666_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 100667_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100667_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100668_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100668_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100672_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100672_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100675_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100675_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 100677_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100677_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 100679_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100679_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 100680_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100680_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100681_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100681_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100685_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100685_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100689_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100689_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 100690_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100690_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100692_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100692_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100693_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100693_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100697_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100697_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100699_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100699_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100700_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100700_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:06:34.91 +26:08:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.724 681985384347314816 121.64559763413 +26.14617583666 13.3410 12.9851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100705_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100705_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:00:22.32 +25:02:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.456 681440958589438208 120.09313970338 +25.04836566967 13.2606 12.8775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100707_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100707_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100709_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100709_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100713_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100713_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:55:35.68 +18:19:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.540 668470393576700544 118.89882454892 +18.32406280184 13.2456 12.7354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100714_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100714_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:56.99 +26:00:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.478 874825056547181952 116.73744817705 +26.00989514308 13.2362 12.7354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100716_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100716_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 100717_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100717_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:13:02.78 +17:59:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.729 657260498871792768 123.26179285773 +17.99737996460 13.6893 13.0206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100718_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100718_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100719_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100719_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 100722_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100722_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100723_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100723_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100725_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100725_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100726_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100726_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100728_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100728_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100730_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100730_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 100734_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100734_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:00:40.80 +17:17:31.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100735_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100735_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:02.89 +18:11:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.675 671226048890627840 116.51220667141 +18.18440853449 13.3201 12.9782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100738_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100738_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 100740_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100740_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100741_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100741_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100742_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100742_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100745_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100745_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 100747_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100747_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100749_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100749_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:33:21.01 +20:21:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.070 663084165287534080 128.33775852926 +20.36373977369 13.5259 13.0722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100751_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100751_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:14:21.04 +17:05:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.414 656593060954459136 123.58741080068 +17.08719620070 13.9178 13.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100754_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100754_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 100757_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100757_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100759_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100759_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100761_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100761_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 100762_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100762_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100763_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100763_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100768_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100768_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:13:35.66 +23:07:39.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100769_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100769_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100771_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100771_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100773_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100773_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 100774_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100774_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100776_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100776_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100783_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100783_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100784_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100784_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:09:00.31 +27:02:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.856 683557587191555200 122.25082345468 +27.03960875676 13.7805 13.1445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100786_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100786_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:10:29.20 +25:31:53.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100788_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100788_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 100791_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100791_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 100799_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100799_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:23:23.69 +21:50:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.684 676272154431156992 125.84875613622 +21.83956531206 13.7950 13.0190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100800_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100800_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 100801_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100801_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 100804_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100804_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 100806_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100806_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:56:43.54 +26:07:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.980 873907239216766464 119.18111346602 +26.12194833225 13.8521 13.1889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100808_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100808_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100809_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100809_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 100810_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100810_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 100813_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100813_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100815_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100815_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 100816_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100816_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100817_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100817_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100818_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100818_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 100829_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100829_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:41:54.11 +17:05:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.270 658434846008647424 130.47580318869 +17.08898537349 14.1373 13.6720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100833_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100833_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 100841_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100841_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100844_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100844_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100845_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100845_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 100846_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100846_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:15:44.04 +18:57:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.276 657445938380109184 123.93339444034 +18.94945917561 14.4018 13.8379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100847_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100847_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100848_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100848_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 100850_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100850_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:40:29.07 +25:01:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.183 690590716398767616 130.12208579036 +25.01904018981 14.6692 14.1948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100854_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100854_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 100855_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100855_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:27:05.26 +17:31:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.789 662082956871571712 126.77198584034 +17.52901311268 14.2370 13.7647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100857_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100857_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100858_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100858_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100863_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100863_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100864_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100864_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:06:10.62 +25:28:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 3.688 681879251411481728 121.54505648393 +25.47205701340 14.4969 14.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100866_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100866_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100868_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100868_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:17:15.50 +21:38:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.523 676402996310610560 124.31412828477 +21.64787214991 14.3638 13.7566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100869_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100869_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100873_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100873_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 100875_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100875_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100884_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100884_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100890_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100890_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 100891_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100891_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100898_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100898_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 100904_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100904_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 100905_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100905_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100907_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100907_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100921_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100921_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 100922_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100922_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 100932_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100932_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 100933_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 100933_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 100939_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100939_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 100947_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 100947_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 101003_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 101003_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 04842_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 04842_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:49:58.82 +26:17:47.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)
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Considering the candidate 54049_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 54049_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 07:46:31.73 +17:12:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.549 668100648432103296 116.63153954194 +17.20994476646 13.3746 12.9058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96406_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 96406_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 68829_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 68829_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 37351_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 37351_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 15495_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 15495_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 73108_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 73108_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:35:46.19 +18:53:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10189_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 10189_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 05529_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
Preparing report for the candidate 05529_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
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Considering the candidate 44370_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 44370_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
**** FOUND 08:51:17.05 +21:17:60.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 70041_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 70041_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 54175_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039
The candidate 54175_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039 did not pass the final checks
