This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi
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
Gaia DR3 2191002386946916352,2461126.9437,11.84,0.05,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 2191002386946916352 20260327.4437 11.84CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:07.82 +57:28:00.1 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2182515776388198784,2461126.9437,13.57,0.05,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 2182515776388198784 20260327.4437 13.57CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:06.99 +53:45:11.2 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4437 2461126.9437 13.17 20:32:32.12 +54:58:08.5
91.23390 8.93193 galactic Cyg Second-epoch detections are separated by 5.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J308.1177+54.9675 | 20:32:32.12 +54:58:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J308.1177+54.9675,2461126.9437,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J308.1177+54.9675 20260327.4437 13.17CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:32.12 +54:58:08.5 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4437 2461126.9437 12.90 21:39:26.00 +52:45:07.0
96.20039 0.14518 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.8611+52.7592 | 21:39:26.00 +52:45:07.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.8611+52.7592,2461126.9437,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.8611+52.7592 20260327.4437 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:26.00 +52:45:07.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4437 2461126.9437 13.29 21:01:33.78 +57:29:38.6
95.75178 7.31672 galactic Cep Second-epoch detections are separated by 2.8" and 5.3 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 | 21:01:33.78 +57:29:38.6 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.048 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9437,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4437 13.29CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:33.78 +57:29:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_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
ZTF J210811.50+522234.3,2461126.9437,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210811.50+522234.3 20260327.4437 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:12.18 +52:22:37.2 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_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 5856025,2461126.9437,10.58,0.05,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 5856025 20260327.4437 10.58CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:27.75 +50:48:13.9 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_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 5846660,2461126.9437,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5846660 20260327.4437 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:18.42 +53:24:09.3 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4437 2461126.9437 12.44 20:31:04.30 +51:01:15.9
87.86140 6.81633 galactic Cyg Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J307.7539+51.0306 | 20:31:04.30 +51:01:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (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
ATO J307.7539+51.0306,2461126.9437,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.7539+51.0306 20260327.4437 12.44CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:31:04.30 +51:01:15.9 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_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 5969818,2461126.9437,13.02,0.05,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
NSVS 5969818 20260327.4437 13.02CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:56.60 +51:18:14.8 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2178108452759109760,2461126.9437,13.29,0.05,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 2178108452759109760 20260327.4437 13.29CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:23.03 +56:34:49.8 ;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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2198970826901267072,2461126.9437,13.14,0.05,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 2198970826901267072 20260327.4437 13.14CV 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:33.66 +56:29:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20_00sec_-14_90C_LIGHT_0496_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20_00sec_-15_00C_LIGHT_0495_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.94402115 27.03.2026 10:39:13.427 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 7 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): 23178
Objects passed selection criteria: 23084
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 18364
Average stars matched: 17154.2 (93.4124 %)
Memory usage VmPeak: 126892 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:04:00 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.94402115 27.03.2026 10:39:13.427 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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: 56 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): 151349
Objects passed selection criteria: 150985
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 113158
Average stars matched: 105507 (93.2388 %)
Memory usage VmPeak: 2632424 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:07:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.94347731
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:23.985 +53:58:03.71
Angular distance between the image centers 0.04 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:27.205 +53:57:58.60
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 21:10:23.985 +53:58:03.71
Second-epoch second image center 21:10:27.205 +53:57:58.60
Angular distance between the image centers 0.00802 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.wkxR6gasdI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.eWQkQh5RMt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits &> /tmp/tmp.Jt7weVtMmL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits &> /tmp/tmp.IVOdvJGsu4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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 13689 out of 25856 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.933084
a=0.000000 b=1.000000 c=22.933084
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.4 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
5.1 pix fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
3.9 pix fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
14.2 mag. fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
14.4 mag. fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wkxR6gasdI (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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3218, passed=25856
Got 25856 stars (including 22610 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 25856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.eWQkQh5RMt (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/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3203, passed=25854
Got 25854 stars (including 22628 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 25854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 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_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.Jt7weVtMmL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1179, passed=18237
Got 18237 stars (including 17057 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat
util/solve_plate_with_UCAC5 got 18237 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 955 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.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.IVOdvJGsu4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1352, passed=20353
Got 20353 stars (including 18994 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat
util/solve_plate_with_UCAC5 got 20353 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 958 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out31397.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31397_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 31397_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33180_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 33180_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:35:55.40 +54:49:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33663_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 33663_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:27:17.71 +53:06:58.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33862_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 33862_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:44:45.09 +53:16:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34120_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 34120_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:20:14.52 +53:01:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34192_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 34192_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:32:02.15 +50:35:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03307_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 03307_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:45:21.49 +57:34:39.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23987_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 23987_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:01:06.80 +50:07:59.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cyg-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 ####
21:16:07.82 +57:28:00.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:23.985 +53:58:03.71
Angular distance between the image centers 0.04 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 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:27.205 +53:57:58.60
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 21:10:23.985 +53:58:03.71
Second-epoch second image center 21:10:27.205 +53:57:58.60
Angular distance between the image centers 0.00802 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.zau5xr9mKX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.wsMwDqhWm2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits &> /tmp/tmp.jA7mROVmGE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits &> /tmp/tmp.53UfyIkFaE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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 14463 out of 180620 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756732
a=0.000000 b=1.000000 c=22.756732
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
5.1 pix fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
3.8 pix fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Limiting magnitude estimates:
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
14.3 mag. fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
14.5 mag. fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.5 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zau5xr9mKX (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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=28755, passed=180569
Got 180569 stars (including 151468 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 180569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.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.wsMwDqhWm2 (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/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=29011, passed=181061
Got 181061 stars (including 151708 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 181061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.51"
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 975 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: 0.50"
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_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.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.jA7mROVmGE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=11341, passed=77507
Got 77507 stars (including 66131 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat
util/solve_plate_with_UCAC5 got 77507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 967 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.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.53UfyIkFaE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=13214, passed=99144
Got 99144 stars (including 85850 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat
util/solve_plate_with_UCAC5 got 99144 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.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_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-38-26_20.00sec_-15.00C_LIGHT_0495.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-02-Q2b1x1_070146_TTUQ2b1x1_18306_5JxxGkOi/wcs_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out174945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out192109.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out109014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out214077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92208.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 205804_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205804_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:13:02.98 +50:08:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.939 2166112540374150656 318.26143947176 +50.14999600779 13.6194 12.8028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205809_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205809_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:57:16.72 +53:50:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.963 2182706949676624512 314.31957623773 +53.84237608798 12.9131 11.9067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205816_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205816_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:52:34.36 +56:04:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.111 2189879240120869632 313.14221883332 +56.08003093271 13.3671 12.7025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205820_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205820_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:43:33.61 +51:55:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.789 2182082568814813568 310.88933180013 +51.91798501352 12.9164 12.0233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205822_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 205822_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 205824_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205824_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:30:25.09 +55:05:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.204 2177572367809755136 322.60539829653 +55.08710401364 13.2609 12.4875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205829_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205829_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:39:51.40 +51:29:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.498 2180736521756288000 309.96471768086 +51.49748691140 13.6607 13.1562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205845_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205845_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:38:50.26 +53:06:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 205848_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205848_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:31:07.65 +51:27:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205862_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205862_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:50:17.07 +57:26:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.463 2190206928944775296 312.56882272247 +57.43862614324 12.8046 11.7965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205878_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205878_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:31:30.85 +54:16:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 205885_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205885_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:37:18.47 +49:36:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.384 1979104682158393216 324.32636562727 +49.60884422090 12.2692 11.1228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205887_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 205887_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:37:52.98 +51:04:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208772_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 208772_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:39:11.99 +57:29:57.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 208936_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 208936_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:27:54.45 +53:19:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210618_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 210618_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:43:19.06 +52:26:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210958_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 210958_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:44:12.88 +55:24:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211538_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 211538_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:50:07.06 +56:48:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211572_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 211572_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:40:02.93 +53:59:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211756_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 211756_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:31:25.59 +49:35:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212547_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 212547_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:11:20.69 +54:26:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212812_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 212812_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:36:51.67 +52:56:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212840_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 212840_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:20:13.90 +56:31:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212859_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 212859_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:43:49.25 +56:55:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213055_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 213055_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:32:30.37 +54:57:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213133_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 213133_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:13:24.04 +58:02:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213306_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 213306_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:51:18.43 +57:35:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213603_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 213603_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:44:23.18 +51:25:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214077_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 214077_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 215033_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 215033_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:05:38.84 +52:38:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215062_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 215062_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:03:54.87 +55:27:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215088_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 215088_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:37:34.44 +54:00:52.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 215585_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 215585_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:25:08.52 +52:27:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215732_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 215732_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:46:38.95 +50:04:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216234_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 216234_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:32:47.90 +51:13:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:26:54.59 +57:22:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:01:06.80 +50:07:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92208_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 92208_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:13:05.52 +50:25:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:32:45.25 +54:17:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56363_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 56363_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:49:19.97 +54:30:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:23:29.96 +52:31:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79640_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 79640_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:05:22.79 +54:03:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:42:03.82 +56:54:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24968_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 24968_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 109014_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 109014_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:24:40.26 +57:18:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174945_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 174945_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:48:15.84 +50:11:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:35:55.40 +54:49:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64691_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 64691_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:51:27.50 +53:56:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143451_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 143451_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 91365_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 91365_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:47:52.62 +53:54:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144740_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 144740_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:04:55.00 +51:34:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192818_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 192818_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 29092_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 29092_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 192373_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 192373_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:45:42.07 +53:32:44.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 192109_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 192109_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:51:35.45 +53:30:17.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 89843_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 89843_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:10:15.90 +53:33:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38067_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 38067_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:02:09.34 +56:40:11.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41670_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 41670_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:44:22.69 +56:29:16.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25766_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
Preparing report for the candidate 25766_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
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Considering the candidate 24538_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 24538_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 20:45:21.49 +57:34:39.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15988_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 15988_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:38:57.78 +57:29:23.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37004_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 37004_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks
**** FOUND 21:52:01.21 +55:47:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177065_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496
The candidate 177065_fd_Cyg-02-Q2b1x1_2026-03-27_05-39-13_20.00sec_-14.90C_LIGHT_0496 did not pass the final checks