This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7
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
target,2461126.8849,5.72,0.05,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 20260327.3849 5.72CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:03.80 +38:46:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3849 2461126.8849 12.64 20:13:32.59 +39:24:42.4
76.51293 2.77410 galactic Cyg Second-epoch detections are separated by 6.3" and 5.2 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 J303.3868+39.4143 | 20:13:32.59 +39:24:42.4 (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 J303.3868+39.4143,2461126.8849,12.64,0.05,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 J303.3868+39.4143 20260327.3849 12.64CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:32.59 +39:24:42.4 ;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-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2067628699755712896,2461126.8849,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2067628699755712896 20260327.3849 12.36CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:42.27 +40:56:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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,2461126.8849,11.79,0.05,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 20260327.3849 11.79CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:36.73 +35:01:42.9 ;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-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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 8511482,2461126.8849,11.72,0.05,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 8511482 20260327.3849 11.72CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:29.08 +36:51:53.9 ;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-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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 J2110193+394032,2461126.8849,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2110193+394032 20260327.3849 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:18.91 +39:40:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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
V1800 Cyg,2461126.8849,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1800 Cyg 20260327.3849 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:03:03.41 +37:48:32.9 ;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-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203904.60+334942.3,2461126.8849,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203904.60+334942.3 20260327.3849 12.36CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:04.08 +33:49:51.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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
V1804 Cyg,2461126.8849,11.78,0.05,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
V1804 Cyg 20260327.3849 11.78CV 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:29.21 +37:10:40.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20_00sec_-14_90C_LIGHT_0400_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: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461126.88515447 27.03.2026 09:14:27.346 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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: 6 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): 25130
Objects passed selection criteria: 24988
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: 17096
Average stars matched: 16057.8 (93.9269 %)
Memory usage VmPeak: 128836 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 05:28:42 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: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461126.88515447 27.03.2026 09:14:27.346 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 44 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): 166772
Objects passed selection criteria: 166212
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 111473
Average stars matched: 104942 (94.1412 %)
Memory usage VmPeak: 1928232 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 05:32:58 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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: 2461126.88463506
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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
Saving wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits to local_wcs_cache/
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits exists and is non-empty
Saving wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits to local_wcs_cache/
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits exists and is non-empty
Saving wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits to local_wcs_cache/
'wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits'
wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits exists and is non-empty
Saving wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:43:33.408 +37:56:34.51
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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:43:34.091 +37:56:11.63
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 20:43:33.408 +37:56:34.51
Second-epoch second image center 20:43:34.091 +37:56:11.63
Angular distance between the image centers 0.00674 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.UhyMQpeX6q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits &> /tmp/tmp.1wyuH9Xk6z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits &> /tmp/tmp.n2vcSGl0Xo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.wBlHi8H0Sn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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 20549 out of 30368 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925229
a=0.000000 b=1.000000 c=22.925229
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
2.4 pix Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
4.2 pix fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
4.0 pix fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Limiting magnitude estimates:
14.8 mag. Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
14.8 mag. Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
13.4 mag. fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
13.4 mag. fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.9 (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.UhyMQpeX6q (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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3799, passed=30368
Got 30368 stars (including 26521 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 30368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 945 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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.1wyuH9Xk6z (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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3780, passed=30367
Got 30367 stars (including 26553 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 30367 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 953 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.55"
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_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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.n2vcSGl0Xo (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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=590, passed=10925
Got 10925 stars (including 10334 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 10925 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 914 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: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.94"
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 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.95"
Estimated accuracy of the plate solution: 1.07"
Excluding outliers - 904 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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.wBlHi8H0Sn (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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=486, passed=10931
Got 10931 stars (including 10439 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 10931 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 917 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: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
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 918 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: 1.07"
Excluding outliers - 907 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
Saving fully-calibrated image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits'
Preparing the HTML report for the field Cyg-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out09634.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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 52385_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 52385_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:04:17.02 +37:51:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50065_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 50065_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:03:04.72 +39:12:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05189_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 05189_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:27:23.26 +41:04:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16280_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 16280_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:12:42.60 +36:44:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13156_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 13156_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:43:41.10 +38:09:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18205_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 18205_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:24.80 +36:29:29.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22500_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 22500_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:33:54.68 +35:15:05.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24801_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 24801_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:11.11 +34:22:28.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 04306_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 04306_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:57:10.78 +41:10:00.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 25882_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 25882_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:46:13.79 +33:58:27.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 09634_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 09634_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06790_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 06790_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:22:14.58 +40:15:22.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 23458_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 23458_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:18:39.42 +34:58:59.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13283_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 13283_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:17:47.71 +38:01:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17295_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 17295_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:14:32.54 +36:48:25.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Cyg-06-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 ####
21:07:03.80 +38:46:10.8
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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Creating symlink local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits exists and is non-empty
wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:43:33.408 +37:56:34.51
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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:43:34.091 +37:56:11.63
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 20:43:33.408 +37:56:34.51
Second-epoch second image center 20:43:34.091 +37:56:11.63
Angular distance between the image centers 0.00674 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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.8QwDeqR29a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits &> /tmp/tmp.sqXqoyGYGD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits &> /tmp/tmp.as7XOsxY9y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.BE9Bb4uqol
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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 22825 out of 208031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749343
a=0.000000 b=1.000000 c=22.749343
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 66 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
2.2 pix Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
4.2 pix fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
4.1 pix fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Limiting magnitude estimates:
15.0 mag. Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
15.0 mag. Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
13.4 mag. fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
13.4 mag. fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 12.7 (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.8QwDeqR29a (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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=36025, passed=207975
Got 207975 stars (including 171588 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 207975 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 944 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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.sqXqoyGYGD (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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=35365, passed=205095
Got 205095 stars (including 169388 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 205095 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 946 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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.as7XOsxY9y (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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5049, passed=55488
Got 55488 stars (including 50403 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 55488 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 914 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: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
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 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 1.06"
Excluding outliers - 904 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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.BE9Bb4uqol (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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4595, passed=55546
Got 55546 stars (including 50904 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 55546 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 915 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: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.88"
Estimated accuracy of the plate solution: 1.08"
Excluding outliers - 904 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Saving fully-calibrated image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-13-42_20.00sec_-14.90C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.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-06-Q2b1x1_052539_TTUQ2b1x1_14352_UKddz5e7/wcs_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401.fits
Preparing the HTML report for the field Cyg-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out232409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89406.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 232409_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 232409_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:23:37.35 +34:01:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.994 2056204499071526400 305.90657785690 +34.03040015705 12.8737 12.4171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 232410_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 232410_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:35:46.71 +36:43:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.204 2062941133790320000 308.94573100175 +36.72688638514 11.9441 10.6436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 232420_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 232420_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:16:54.77 +39:49:21.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 232426_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 232426_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:14:42.58 +38:52:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232428_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 232428_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:15:48.49 +35:59:49.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
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Considering the candidate 232430_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 232430_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 232442_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 232442_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 235488_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 235488_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:04:42.60 +41:12:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235884_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 235884_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:46:20.51 +34:01:00.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 237012_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 237012_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:17:42.30 +38:00:22.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 237353_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 237353_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:46:59.70 +34:22:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237488_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 237488_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:22:58.77 +40:46:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 3.660 2067570391280387456 305.74357907928 +40.77043196707 11.9611 11.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 238342_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 238342_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:12:59.23 +40:08:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238626_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 238626_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:51:33.20 +39:24:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238804_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 238804_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:06:32.77 +37:32:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 238880_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 238880_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:58:32.96 +41:22:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239686_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 239686_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:02:15.17 +39:29:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.038 1872982293739150592 315.56254671518 +39.48818916109 11.9067 10.9947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 241736_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 241736_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:41:30.84 +36:38:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197574_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 197574_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 118564_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 118564_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 172936_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 172936_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:41:45.62 +33:53:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117778_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 117778_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:01:41.54 +36:36:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132183_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 132183_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:52:03.09 +36:07:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200042_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 200042_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:46:37.72 +34:59:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142515_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 142515_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:56.50 +35:44:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49182_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 49182_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 149510_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 149510_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:27:37.11 +35:33:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118361_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 118361_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:45:11.06 +36:48:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89584_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 89584_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:43:41.10 +38:09:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89406_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 89406_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 110702_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 110702_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:12:42.60 +36:44:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171550_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 171550_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 185818_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 185818_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:43:50.72 +34:28:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101123_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
Preparing report for the candidate 101123_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
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Considering the candidate 199860_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 199860_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:36:11.79 +35:07:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183224_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 183224_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:43.24 +34:19:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88862_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 88862_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:04:17.01 +37:51:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60176_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 60176_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:03:04.64 +39:12:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32936_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 32936_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:27:23.29 +41:04:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13820_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 13820_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:11:36.19 +41:51:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86558_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 86558_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:37:23.82 +38:19:43.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129368_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 129368_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:24.48 +36:29:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 150139_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 150139_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:49:12.32 +35:33:47.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 120482_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 120482_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:30:59.45 +36:56:09.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41234_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 41234_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:39:33.59 +40:34:43.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152836_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 152836_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:57:12.74 +35:18:45.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 84568_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 84568_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:27:34.37 +38:26:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130891_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 130891_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:29:20.67 +36:27:18.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56208_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 56208_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:02:21.00 +39:30:32.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 72674_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 72674_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:03:04.94 +38:39:26.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201485_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 201485_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:33:54.66 +35:15:05.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 184909_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 184909_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:47:11.09 +34:22:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 134319_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 134319_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:01:12.96 +36:01:33.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23292_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 23292_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:41:56.85 +41:43:01.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105555_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 105555_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:23:44.54 +37:28:36.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 158047_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 158047_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:46:13.78 +33:58:27.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 179679_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 179679_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:27:07.87 +34:19:44.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29821_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 29821_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:57:10.77 +41:10:00.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70544_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 70544_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:07:03.96 +38:46:14.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 49535_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 49535_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:22:14.56 +40:15:22.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 113346_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 113346_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 21:13:26.37 +36:37:56.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 35051_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 35051_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:22:45.68 +41:01:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118149_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 118149_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:18:29.02 +37:00:01.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 93459_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 93459_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:17:47.69 +38:01:60.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195621_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 195621_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks
**** FOUND 20:18:39.39 +34:58:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120433_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401
The candidate 120433_fd_Cyg-06-Q2b1x1_2026-03-27_04-14-27_20.00sec_-15.00C_LIGHT_0401 did not pass the final checks