This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC
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
KIC 3437693,2461126.8462,12.36,0.05,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
KIC 3437693 20260327.3462 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:07.46 +38:33:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_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 2047752587561466496,2461126.8462,11.79,0.05,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
Gaia DR3 2047752587561466496 20260327.3462 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:08.88 +35:15:24.6 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3462 2461126.8462 11.56 19:59:49.91 +37:54:10.5
73.79885 4.22372 galactic Cyg Second-epoch detections are separated by 1.3" and 38.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9600+37.8962 | 19:59:49.18 +37:54:09.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9600+37.8962,2461126.8462,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9600+37.8962 20260327.3462 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:49.91 +37:54:10.5 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3462 2461126.8462 12.04 19:06:43.32 +38:18:56.7
69.25855 13.66081 galactic Lyr Second-epoch detections are separated by 1.8" and 36.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2099229449911277056 | 19:06:44.23 +38:19:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2099229449911277056,2461126.8462,12.04,0.05,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 2099229449911277056 20260327.3462 12.04CV 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:43.32 +38:18:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_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
V0497 Lyr,2461126.8462,12.52,0.05,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
V0497 Lyr 20260327.3462 12.52CV 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:07:49.34 +36:23:08.6 ;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-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3462 2461126.8462 12.44 19:06:04.62 +35:56:18.7
66.97647 12.80473 galactic Lyr Second-epoch detections are separated by 2.5" and 36.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.5148+35.9381 | 19:06:04.62 +35:56:18.7 (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 J286.5148+35.9381,2461126.8462,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.5148+35.9381 20260327.3462 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:04.62 +35:56:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_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
HAT 199-04294,2461126.8462,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04294 20260327.3462 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:21.97 +41:02:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_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 2047218461112031104,2461126.8462,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2047218461112031104 20260327.3462 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:27.00 +34:16:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20_00sec_-14_90C_LIGHT_0347_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20_00sec_-15_00C_LIGHT_0337_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: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461126.85197024 27.03.2026 08:26:40.229 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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): 27658
Objects passed selection criteria: 27531
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: 19306
Average stars matched: 18650.8 (96.606 %)
Memory usage VmPeak: 133520 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 03:30:29 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: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461126.85197024 27.03.2026 08:26:40.229 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 120
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 42 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): 235090
Objects passed selection criteria: 234332
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 154235
Average stars matched: 147333 (95.525 %)
Memory usage VmPeak: 2884168 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 03:36:26 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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: 2461126.84049972
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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
Saving wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits to local_wcs_cache/
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits'
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits'
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:06.178 +37:55:25.23
Angular distance between the image centers 0.09 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:05.491 +37:59:05.67
Angular distance between the image centers 0.06 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 19:38:06.178 +37:55:25.23
Second-epoch second image center 19:38:05.491 +37:59:05.67
Angular distance between the image centers 0.06128 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.02g3wlNSth
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.wSOqvR6uhS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits &> /tmp/tmp.eF53G8VBlr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits &> /tmp/tmp.YUgbsGMkkW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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 2233 out of 36462 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.855034
a=0.000000 b=1.000000 c=22.855034
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
2.2 pix Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
5.0 pix fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
4.2 pix fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Limiting magnitude estimates:
15.0 mag. Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.0 mag. Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
13.0 mag. fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
13.6 mag. fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.6 (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.02g3wlNSth (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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4454, passed=36462
Got 36462 stars (including 31968 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 36462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 851 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: 2.11"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.34"
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 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.31"
Estimated accuracy of the plate solution: 1.31"
Excluding outliers - 896 stars left (next iteration limit 907)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.wSOqvR6uhS (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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4450, passed=36391
Got 36391 stars (including 31905 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 36391 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 920 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: 2.11"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.16"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.13"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 912 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.eF53G8VBlr (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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=225, passed=7353
Got 7353 stars (including 7127 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat
util/solve_plate_with_UCAC5 got 7353 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 931 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: 1.11"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.09"
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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.10"
Estimated accuracy of the plate solution: 1.25"
Excluding outliers - 920 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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.YUgbsGMkkW (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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=537, passed=12735
Got 12735 stars (including 12196 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 12735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 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: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.87"
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 930 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
Saving fully-calibrated image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits'
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits exists and is non-empty
wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits exists and is non-empty
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:06.178 +37:55:25.23
Angular distance between the image centers 0.09 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:05.491 +37:59:05.67
Angular distance between the image centers 0.06 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 19:38:06.178 +37:55:25.23
Second-epoch second image center 19:38:05.491 +37:59:05.67
Angular distance between the image centers 0.06128 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.9OiZ1Bu5yK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.T3IoZ7Trop
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits &> /tmp/tmp.BgXRB4WdLr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits &> /tmp/tmp.d8SGbDr5IO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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 2470 out of 289933 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.659513
a=0.000000 b=1.000000 c=22.659513
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 91 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
1.9 pix Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
5.1 pix fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
4.3 pix fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Limiting magnitude estimates:
15.2 mag. Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.2 mag. Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
13.0 mag. fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
13.6 mag. fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.3 (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.9OiZ1Bu5yK (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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=54567, passed=289884
Got 289884 stars (including 234962 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 289884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 835 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: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.33"
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 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.33"
Estimated accuracy of the plate solution: 1.37"
Excluding outliers - 887 stars left (next iteration limit 889)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.T3IoZ7Trop (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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=55059, passed=293495
Got 293495 stars (including 238063 good ones) from the SExtractor catalog wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 293495 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 889 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: 2.07"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.15"
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 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.14"
Estimated accuracy of the plate solution: 1.22"
Excluding outliers - 897 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.BgXRB4WdLr (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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3363, passed=41110
Got 41110 stars (including 37726 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat
util/solve_plate_with_UCAC5 got 41110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (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 0.010434 (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 928 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: 1.13"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.06"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.07"
Estimated accuracy of the plate solution: 1.24"
Excluding outliers - 918 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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.d8SGbDr5IO (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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Checking if the catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat corresponding to the image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
WCS catalog name: wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=6762, passed=70619
Got 70619 stars (including 63823 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat
util/solve_plate_with_UCAC5 got 70619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.83"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.83"
Estimated accuracy of the plate solution: 1.06"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits -region wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Saving fully-calibrated image wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-10-09_20.00sec_-15.00C_LIGHT_0337.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.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-05-Q2b1x1_032809_TTUQ2b1x1_6404_qPw4XmDC/wcs_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347.fits
Preparing the HTML report for the field Cyg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out302575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out114759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45077.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 325969_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325969_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:33:24.49 +37:42:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.214 2051665096597610496 293.35174503847 +37.71334096734 12.6882 12.2423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 325979_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325979_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:45:43.13 +34:54:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.031 2047532891406661632 296.42956355360 +34.90746150526 12.0260 11.6354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 325980_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325980_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:57:43.48 +34:36:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.269 2059292443128283392 299.43131760543 +34.60328119457 11.5636 10.6338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 325984_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325984_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 20:02:58.57 +41:05:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.669 2074416088131126912 300.74380540181 +41.08619687403 10.3999 8.8872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 325985_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 325985_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 325991_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325991_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:51:41.60 +37:54:35.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)
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Considering the candidate 325992_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325992_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:59:53.55 +36:16:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 325994_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 325994_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:11:45.92 +41:52:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.095 2102398723462571776 287.94094016131 +41.87864174606 11.9969 11.3155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 325998_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 325998_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 326004_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 326004_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 326008_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 326008_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:56:40.43 +39:19:43.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)
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Considering the candidate 326012_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 326012_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:28:53.59 +34:08:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 1.994 2046647058659746560 292.22395792130 +34.13605226608 11.8362 11.1450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 326511_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 326511_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:50:48.20 +37:51:43.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 326672_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 326672_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:43:13.22 +40:01:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122586_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 122586_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:07:18.22 +36:06:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99753_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 99753_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 20:00:13.38 +36:08:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187381_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 187381_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 61065_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 61065_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:31:31.49 +34:42:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188769_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 188769_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:51:49.08 +39:00:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233771_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 233771_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:47:34.84 +40:44:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232006_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 232006_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:19:53.74 +40:15:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127418_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 127418_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 50682_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 50682_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:09:26.99 +33:56:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157116_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 157116_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 20:07:57.31 +37:57:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 276789_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 276789_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:20:08.91 +41:40:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 222848_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 222848_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:45:26.13 +40:15:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114759_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 114759_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 120666_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 120666_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:40:59.12 +36:43:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51759_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 51759_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:40:55.39 +34:31:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210606_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 210606_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:44:09.73 +39:47:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248978_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 248978_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 216463_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 216463_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:41:31.33 +40:00:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45077_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
Preparing report for the candidate 45077_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
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Considering the candidate 60849_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 60849_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:15:56.47 +34:27:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181644_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 181644_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:37:17.60 +38:35:39.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 113768_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 113768_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:25:58.07 +36:11:11.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 174982_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 174982_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:36:56.71 +38:23:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 187223_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 187223_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:33:36.50 +38:45:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218704_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 218704_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:41:39.73 +40:01:23.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 220754_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 220754_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:28:38.52 +39:56:26.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 214428_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 214428_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:23:47.81 +39:35:26.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 182674_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 182674_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:43:10.78 +38:40:18.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 235937_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 235937_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:42:56.31 +40:43:18.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 131788_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 131788_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:35:48.42 +36:56:42.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 146804_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 146804_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:25:18.20 +37:14:42.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 76844_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 76844_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:36:07.47 +35:12:47.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 113368_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 113368_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:29:29.87 +36:17:21.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 167683_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 167683_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:27:36.45 +37:56:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173848_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 173848_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:47:27.76 +38:24:32.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79348_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 79348_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:38:01.51 +35:15:31.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 226310_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 226310_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:41:57.54 +40:15:19.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75892_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 75892_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:48:43.86 +35:18:43.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110717_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 110717_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:30:46.93 +36:13:42.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 224429_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 224429_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:20:27.19 +39:55:33.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 182268_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 182268_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:49:27.46 +38:42:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101247_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 101247_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:45:39.94 +36:05:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173898_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 173898_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:57:29.02 +38:27:30.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 159231_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 159231_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:50:46.91 +37:49:35.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 158446_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 158446_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:22:40.95 +37:34:53.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 123604_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 123604_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:24:06.15 +36:27:09.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 72044_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 72044_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:37:40.84 +35:01:22.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 276093_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 276093_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:34:18.12 +41:55:38.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 111692_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 111692_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:52:16.44 +36:25:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203867_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 203867_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:17:09.20 +39:01:44.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 236846_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 236846_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:44:48.98 +40:42:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68745_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 68745_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:45:51.42 +35:00:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117634_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 117634_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:26:09.35 +36:19:05.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 221701_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 221701_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:55:40.52 +40:10:24.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 35843_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 35843_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:30:17.32 +33:43:42.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 129101_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 129101_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:54:48.24 +36:59:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 162764_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 162764_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:58:34.43 +38:06:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151718_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 151718_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:19:38.92 +37:19:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 232930_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 232930_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:50:37.43 +40:36:00.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155919_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 155919_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:19:01.18 +37:26:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 205351_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 205351_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:17:20.05 +39:07:15.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 38771_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 38771_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:39:44.83 +33:58:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44456_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 44456_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:43:51.40 +34:09:46.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52283_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 52283_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:44:38.21 +34:24:52.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 36538_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 36538_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:34:56.04 +33:47:46.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 106363_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 106363_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:56:44.16 +36:15:03.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 279687_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 279687_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:43:45.27 +41:46:23.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82510_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 82510_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:20:33.19 +35:11:10.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130322_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 130322_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:59:55.14 +37:02:35.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 131938_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 131938_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 20:01:15.33 +37:05:57.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226806_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 226806_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:57:13.93 +40:22:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107752_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 107752_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:09:56.39 +35:39:40.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 302575_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 302575_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:13:17.82 +37:03:26.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)
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Considering the candidate 174981_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 174981_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 20:05:10.08 +38:28:44.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 275390_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 275390_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:06:16.87 +41:24:50.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74654_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 74654_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks
**** FOUND 19:09:04.14 +34:36:06.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 250232_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347
The candidate 250232_fd_Cyg-05-Q2b1x1_2026-03-27_03-26-40_20.00sec_-14.90C_LIGHT_0347 did not pass the final checks