This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg
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
V1666 Cyg,2461126.9306,11.39,0.05,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
V1666 Cyg 20260327.4306 11.39CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:51.84 +35:20:26.3 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4306 2461126.9306 12.82 21:35:35.27 +39:44:14.2
86.95973 -9.08153 galactic Cyg Second-epoch detections are separated by 0.9" and 7.2 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 J323.8928+39.7362 | 21:35:35.27 +39:44:14.2 (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 J323.8928+39.7362,2461126.9306,12.82,0.05,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 J323.8928+39.7362 20260327.4306 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:35.27 +39:44:14.2 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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
V0386 Peg,2461126.9306,11.96,0.05,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
V0386 Peg 20260327.4306 11.96CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:58.73 +33:48:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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
IL Peg,2461126.9306,11.77,0.05,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
IL Peg 20260327.4306 11.77CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:36.23 +36:23:37.2 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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
ASASSN-V J212906.70+404414.4,2461126.9306,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212906.70+404414.4 20260327.4306 12.43CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:06.43 +40:44:06.9 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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 J2151195+410702,2461126.9306,12.86,0.05,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 J2151195+410702 20260327.4306 12.86CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:51:19.88 +41:07:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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
ASASSN-V J214540.10+383337.6,2461126.9306,12.44,0.05,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
ASASSN-V J214540.10+383337.6 20260327.4306 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:40.12 +38:33:44.9 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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
V0640 Cyg,2461126.9306,11.89,0.05,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
V0640 Cyg 20260327.4306 11.89CV 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:39:16.68 +41:13:38.3 ;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-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9306,12.60,0.05,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 20260327.4306 12.60CV 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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:04.40 +41:58:27.0 ;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-07-Q2b1x1_2025-12-26_19-23-42_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20_00sec_-15_00C_LIGHT_0473_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20_00sec_-15_00C_LIGHT_0472_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: 2461036.55771816 27.12.2025 01:22:56.849 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
First image: 2461036.55771816 27.12.2025 01:22:56.849 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Last image: 2461126.93093693 27.03.2026 10:20:22.951 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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): 20793
Objects passed selection criteria: 20704
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: 15124.5
Average stars matched: 14087.5 (93.1436 %)
Memory usage VmPeak: 125092 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 05:30:08 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: 2461036.55771816 27.12.2025 01:22:56.849 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
First image: 2461036.55771816 27.12.2025 01:22:56.849 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Last image: 2461126.93093693 27.03.2026 10:20:22.951 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 39 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): 139448
Objects passed selection criteria: 139089
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 97770.2
Average stars matched: 91157 (93.2359 %)
Memory usage VmPeak: 1904672 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 05:33:32 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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: 2461126.93032799
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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits'
wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
Saving wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits'
wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits exists and is non-empty
Saving wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits to local_wcs_cache/
'wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits' -> 'local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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 21:49:05.494 +37:59:54.54
Second-epoch image center 21:48:56.663 +37:56:37.67
Angular distance between the image centers 0.06 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 21:49:05.494 +37:59:54.54
Second-epoch image center 21:48:57.107 +37:55:54.56
Angular distance between the image centers 0.07 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 21:48:56.663 +37:56:37.67
Second-epoch second image center 21:48:57.107 +37:55:54.56
Angular distance between the image centers 0.01206 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits &> /tmp/tmp.TYn0aroffl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.kBqGBaIaMQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits &> /tmp/tmp.BiLl9IORFy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits &> /tmp/tmp.9YILTv0BtI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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 15775 out of 25390 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958506
a=0.000000 b=1.000000 c=22.958506
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
2.5 pix Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
5.9 pix fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
3.8 pix fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Limiting magnitude estimates:
15.0 mag. Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
15.0 mag. Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
13.6 mag. fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
14.0 mag. fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TYn0aroffl (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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2586, passed=25390
Got 25390 stars (including 22783 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 25390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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: 0.47"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits -region wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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.kBqGBaIaMQ (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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2616, passed=25299
Got 25299 stars (including 22653 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 25299 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 965 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: 0.47"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.46"
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_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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.BiLl9IORFy (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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=408, passed=9903
Got 9903 stars (including 9492 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat
util/solve_plate_with_UCAC5 got 9903 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 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 956 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: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.95"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.96"
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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.9YILTv0BtI (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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=532, passed=12764
Got 12764 stars (including 12223 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat
util/solve_plate_with_UCAC5 got 12764 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 956 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: 0.79"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits'
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits'
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits'
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out19712.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32030_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 32030_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:51:19.39 +36:49:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32374_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 32374_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:48:31.51 +42:05:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19712_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 19712_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09555_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 09555_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:12:51.27 +39:09:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19019_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 19019_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:42:01.35 +35:30:39.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11768_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 11768_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:34:47.27 +38:32:07.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05456_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 05456_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:43:06.68 +41:09:21.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07361_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 07361_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:36:57.30 +40:24:50.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07898_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 07898_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:13:52.85 +39:42:54.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12625_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 12625_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:15:58.17 +37:44:57.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cyg-07-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 ####
21:26:51.84 +35:20:26.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat to cache
SExtractor catalog cache: saved Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Creating symlink local_wcs_cache/wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits exists and is non-empty
wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits exists and is non-empty
wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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 21:49:05.494 +37:59:54.54
Second-epoch image center 21:48:56.663 +37:56:37.67
Angular distance between the image centers 0.06 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 21:49:05.494 +37:59:54.54
Second-epoch image center 21:48:57.107 +37:55:54.56
Angular distance between the image centers 0.07 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 21:48:56.663 +37:56:37.67
Second-epoch second image center 21:48:57.107 +37:55:54.56
Angular distance between the image centers 0.01206 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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits &> /tmp/tmp.Y4cArSKxpE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.yrfOR3z1W1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits &> /tmp/tmp.LEwTah30nZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits &> /tmp/tmp.GTyWbt7yyB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
Found non-empty wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits and wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
The reference image (wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits) and catalog (wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat) found
'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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 16634 out of 175999 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.782761
a=0.000000 b=1.000000 c=22.782761
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
2.2 pix Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
5.9 pix fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
3.9 pix fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Limiting magnitude estimates:
15.2 mag. Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
15.2 mag. Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
13.7 mag. fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
14.0 mag. fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.0 (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.Y4cArSKxpE (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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=67, blended=24552, passed=175932
Got 175932 stars (including 151084 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 175932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits -region wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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.yrfOR3z1W1 (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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat corresponding to the image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=24644, passed=176102
Got 176102 stars (including 151180 good ones) from the SExtractor catalog wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 176102 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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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.LEwTah30nZ (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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4944, passed=46075
Got 46075 stars (including 41112 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat
util/solve_plate_with_UCAC5 got 46075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 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 958 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: 0.92"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.92"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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.GTyWbt7yyB (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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS-calibrated image found: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Checking if the catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat corresponding to the image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
WCS catalog name: wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=5813, passed=64615
Got 64615 stars (including 58754 good ones) from the SExtractor catalog wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat
util/solve_plate_with_UCAC5 got 64615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 958 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: 0.79"
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 958 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: 0.79"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits -region wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits
Saving fully-calibrated image wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_Cyg-07-Q2b1x1_2025-12-26_19-23-42_20.00sec_-15.00C_LIGHT_0025.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-19-30_20.00sec_-15.00C_LIGHT_0472.fits
Saving fully-calibrated image wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.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-07-Q2b1x1_052740_TTUQ2b1x1_4465_bwP2SxWg/wcs_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473.fits
Preparing the HTML report for the field Cyg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out18538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out120765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82483.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 200060_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200060_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:12:41.95 +41:27:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.141 1958067245129564160 333.17448545293 +41.46405197785 13.0199 12.5597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200072_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200072_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:46:20.34 +41:17:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.498 1954490151547748736 326.58519581395 +41.28938584143 13.0235 12.5083 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 200074_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200074_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:48:15.53 +35:26:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.984 1949242938463110400 327.06469299925 +35.43999539451 12.6888 11.9648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200075_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200075_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:27:50.59 +40:58:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.671 1967028711577959680 321.96083156463 +40.96960055592 12.6551 11.7181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200076_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200076_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:23:55.63 +35:19:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.698 1951489451178833280 320.98270993169 +35.31849362383 12.6312 11.8503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200077_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200077_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:59:47.31 +37:31:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.707 1949752875641928960 329.94767063849 +37.52522274438 13.0391 12.5030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200079_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200079_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:09:02.46 +35:35:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.705 1906507846367940864 332.26058674299 +35.59455300414 12.9512 12.4039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200084_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200084_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:39:40.23 +40:36:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.499 1966398657052906368 324.91690929098 +40.61465140022 13.0792 12.5658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200085_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200085_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:06:21.87 +33:33:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.474 1900041682905296896 331.58996711947 +33.55561841643 12.6983 12.2390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200100_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200100_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:31:35.62 +35:39:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.983 1951380084131769088 322.89777045639 +35.65044458821 12.5081 11.5178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200101_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200101_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:12:14.70 +40:26:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.247 1956456563674914176 333.06006484112 +40.44638270766 12.7886 12.2607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200109_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200109_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:35:48.78 +35:20:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.807 1950927325858171904 323.95469991796 +35.34857465076 13.3362 12.7503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200111_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 200111_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 200119_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200119_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:19:21.07 +38:57:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 200125_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200125_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:26:23.23 +34:48:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.442 1951261061999211776 321.59637311322 +34.80690548423 12.2398 11.5186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200129_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200129_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:41:04.97 +41:56:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200142_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200142_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:28:37.55 +39:25:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 200143_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200143_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:45:59.39 +40:17:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.512 1954232217293151232 326.49738614204 +40.29200020108 12.5564 12.0216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200144_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200144_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:17:50.13 +41:27:32.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
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Considering the candidate 200146_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200146_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:19:23.60 +35:00:28.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 200148_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200148_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:43:34.56 +39:38:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.218 1954101169251299456 325.89356775793 +39.63933863056 10.6347 9.1867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200151_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200151_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:31:34.57 +35:30:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.593 1951354584903460096 322.89526311437 +35.50452399484 12.7555 12.2812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200156_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200156_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 200982_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 200982_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:51:19.41 +36:49:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204836_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 204836_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:11:44.68 +38:23:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205829_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 205829_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:35:04.82 +40:51:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 206075_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 206075_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:45:50.89 +35:50:24.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 206741_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 206741_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:47:46.85 +38:13:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18538_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 18538_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:19:43.75 +41:45:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.089 1957748897854003968 334.93141918508 +41.75601355848 11.9620 11.5568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 165790_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 165790_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 147242_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 147242_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:03:42.46 +35:43:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21570_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 21570_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:48:31.51 +42:05:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137850_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 137850_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:26:51.88 +35:20:27.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 120765_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 120765_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 44910_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 44910_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 37663_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 37663_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 41288_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 41288_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:49:56.77 +40:56:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82483_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 82483_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 66251_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 66251_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:12:51.25 +39:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119855_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 119855_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:56:38.22 +36:20:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37275_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 37275_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 187186_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
Preparing report for the candidate 187186_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
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Considering the candidate 133154_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 133154_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 22:05:42.17 +35:20:54.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 82827_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 82827_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:48:29.56 +38:38:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 89422_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 89422_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:43:25.93 +38:17:02.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66014_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 66014_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:51:05.18 +39:32:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120407_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 120407_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:48:08.50 +36:34:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 146125_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 146125_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:45:44.83 +35:51:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 140795_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 140795_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:42:01.38 +35:30:38.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45919_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 45919_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:41:34.38 +40:48:23.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40505_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 40505_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:43:06.66 +41:09:21.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40789_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 40789_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:42:23.18 +41:04:43.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52865_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 52865_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:36:57.31 +40:24:49.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 109257_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 109257_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:27:21.57 +37:07:03.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117965_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 117965_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks
**** FOUND 21:25:47.13 +36:40:04.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 89597_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473
The candidate 89597_fd_Cyg-07-Q2b1x1_2026-03-27_05-20-22_20.00sec_-15.00C_LIGHT_0473 did not pass the final checks