This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.8623,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.3623 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:55.52 +56:43:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203749.12+512848.3,2461128.8623,13.04,0.05,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
ZTF J203749.12+512848.3 20260329.3623 13.04CV 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:37:48.66 +51:28:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3623 2461128.8623 13.12 20:50:12.52 +56:47:13.1
94.20965 8.04872 galactic Cep Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.5574+56.7912 | 20:50:12.52 +56:47:13.1 (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 J312.5574+56.7912,2461128.8623,13.12,0.05,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 J312.5574+56.7912 20260329.3623 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:50:12.52 +56:47:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_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
NSV 25231,2461128.8623,12.91,0.05,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
NSV 25231 20260329.3623 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:59.87 +49:57:49.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3281971,2461128.8623,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3281971 20260329.3623 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:53.36 +54:35:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214214.23+542136.6,2461128.8623,12.56,0.05,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
ASASSN-V J214214.23+542136.6 20260329.3623 12.56CV 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:13.42 +54:21:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.8623,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.3623 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:35.35 +52:18:40.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3298248,2461128.8623,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3298248 20260329.3623 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:43.88 +51:13:54.7 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5856025,2461128.8623,10.56,0.05,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
NSVS 5856025 20260329.3623 10.56CV 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-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:19:26.54 +50:48:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2100331+500302,2461128.8623,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2100331+500302 20260329.3623 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:33.35 +50:03:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214248.81+563403.1,2461128.8623,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214248.81+563403.1 20260329.3623 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:48.63 +56:33:59.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214614.97+514437.8,2461128.8623,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214614.97+514437.8 20260329.3623 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:14.62 +51:44:37.7 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2148354+572324,2461128.8623,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2148354+572324 20260329.3623 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:35.14 +57:23:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_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
V0480 Cep,2461128.8623,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0480 Cep 20260329.3623 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:07.61 +55:30:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5850227,2461128.8623,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5850227 20260329.3623 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:12:59.69 +50:37:35.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_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
V1088 Cyg,2461128.8623,12.47,0.05,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
V1088 Cyg 20260329.3623 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:42:14.25 +53:04:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212046.13+530618.7,2461128.8623,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212046.13+530618.7 20260329.3623 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:46.14 +53:06:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211828.84+500850.2,2461128.8623,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211828.84+500850.2 20260329.3623 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:28.73 +50:08:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20_00sec_-14_90C_LIGHT_0317_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461128.86258294 29.03.2026 08:41:57.166 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21963
Objects passed selection criteria: 21831
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: 15153.8
Average stars matched: 14256.5 (94.079 %)
Memory usage VmPeak: 126056 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 Sun Mar 29 03:44:13 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461036.55222016 27.12.2025 01:15:01.822 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461128.86258294 29.03.2026 08:41:57.166 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 197
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 34 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): 153326
Objects passed selection criteria: 152934
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: 109180
Average stars matched: 101451 (92.9204 %)
Memory usage VmPeak: 1977060 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 Sun Mar 29 03:46:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.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: 2461128.86196355
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:27.379 +54:00:12.10
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:30.748 +54:00:07.37
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:27.379 +54:00:12.10
Second-epoch second image center 21:10:30.748 +54:00:07.37
Angular distance between the image centers 0.00835 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.ih8BHsO3bY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.4ftWUWHj1u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits &> /tmp/tmp.5neVoo6i7b
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.1V4HWEopKq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 13689 out of 25856 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.933084
a=0.000000 b=1.000000 c=22.933084
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.4 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
2.8 pix fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
2.8 pix fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
14.9 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
13.8 mag. fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
13.9 mag. fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ih8BHsO3bY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3218, passed=25856
Got 25856 stars (including 22610 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 25856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4ftWUWHj1u (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3203, passed=25854
Got 25854 stars (including 22628 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 25854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5neVoo6i7b (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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=705, passed=10379
Got 10379 stars (including 9664 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat
util/solve_plate_with_UCAC5 got 10379 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.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.1V4HWEopKq (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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=694, passed=10446
Got 10446 stars (including 9737 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 963 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 33061_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 33061_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:35:55.08 +54:49:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14271_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 14271_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:23:29.65 +52:31:52.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:27.379 +54:00:12.10
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:36.437 +53:59:53.51
Second-epoch image center 21:10:30.748 +54:00:07.37
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:27.379 +54:00:12.10
Second-epoch second image center 21:10:30.748 +54:00:07.37
Angular distance between the image centers 0.00835 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.dPZYkT2uW4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.uqipXwUwAm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits &> /tmp/tmp.0cqFQVXvK1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.Gy0J4cPoyK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 14463 out of 180620 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756732
a=0.000000 b=1.000000 c=22.756732
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 155 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
2.3 pix Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
2.5 pix fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
2.5 pix fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Limiting magnitude estimates:
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
15.1 mag. Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
14.0 mag. fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
14.0 mag. fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dPZYkT2uW4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=28755, passed=180569
Got 180569 stars (including 151468 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 180569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uqipXwUwAm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=29011, passed=181061
Got 181061 stars (including 151708 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 181061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0cqFQVXvK1 (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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=5367, passed=71288
Got 71288 stars (including 65846 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat
util/solve_plate_with_UCAC5 got 71288 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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 961 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.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.Gy0J4cPoyK (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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5447, passed=71307
Got 71307 stars (including 65775 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 71307 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-49_20.00sec_-15.00C_LIGHT_0017.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-03_20.00sec_-14.90C_LIGHT_0317.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.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_2026-03-29_CI_Cyg-02-Q2b1x1_034247_TTUQ2b1x1_711_GAKfBC7X/wcs_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out192818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out210524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out210633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out216226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out216519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out216647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out214494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out214636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96299.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 8s
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Considering the candidate 205805_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 205805_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205810_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205810_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:33:51.89 +51:57:32.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 205827_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205827_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:31:07.51 +51:27:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205834_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205834_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:03:03.12 +56:04:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.908 2189001589325401728 315.76276599724 +56.07202125804 12.2176 10.8103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205838_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205838_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:29:10.35 +58:05:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205840_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205840_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:41:54.83 +55:25:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205843_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205843_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:58:56.27 +57:29:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.044 2190067905145312768 314.73493502850 +57.49284002362 12.5960 11.4496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205845_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205845_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:37:54.73 +51:03:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205846_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205846_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:30.15 +54:01:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.127 2183425519185741696 308.12603420750 +54.02532727854 13.0369 12.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205847_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205847_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:34:42.92 +49:51:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.189 1979152132959201920 323.67790411545 +49.85827059414 12.0281 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205850_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205850_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:31:35.24 +57:31:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205851_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205851_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:38:30.08 +50:10:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205854_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205854_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:39:16.29 +57:42:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205856_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205856_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:33:42.40 +50:15:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205858_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 205858_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:35:10.63 +50:13:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.944 2171337728873807872 323.79410487559 +50.23133894589 11.8731 10.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207096_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 207096_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:40:33.24 +54:20:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208637_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 208637_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:01:48.84 +57:05:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208981_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 208981_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:03:43.82 +53:15:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209187_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209187_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:39:11.93 +57:29:56.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209189_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209189_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:26.04 +57:45:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.240 2193272672299796224 310.60843323917 +57.75334252127 12.0173 11.0909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209294_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209294_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:39:12.33 +54:30:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.657 2183359548490404480 309.80117990637 +54.51455137951 12.6341 11.7327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209310_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209310_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:17:56.19 +55:15:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209419_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209419_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:29:02.74 +51:14:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209559_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209559_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:54:07.11 +57:09:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.947 2190088250409691136 313.52985725778 +57.16699833237 12.0279 11.2621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209640_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209640_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:38:50.81 +57:27:31.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209979_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 209979_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:27:54.43 +53:19:28.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 210161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:31:13.31 +50:07:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210524_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 210524_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:43:46.91 +49:41:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.420 2168259439910381568 310.94559753101 +49.69265743051 12.3435 12.0137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210533_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 210533_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:32:59.67 +49:57:24.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210633_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 210633_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:50:56.51 +56:56:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.528 2190000147738534272 312.73564643841 +56.94379906020 12.4822 11.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211292_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211292_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:50:06.56 +56:48:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211314_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211314_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:34:52.03 +53:49:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.646 2183410534038731904 308.71803141146 +53.81723723771 12.9360 12.3446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211507_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211507_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:02:21.97 +56:39:57.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211605_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211605_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:44:11.92 +56:27:44.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211814_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211814_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:24.77 +57:23:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.975 2187250440959148416 310.60321585341 +57.39838199330 12.6886 11.9857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211825_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211825_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:53:54.92 +56:20:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.036 2189911744433787136 313.47984946268 +56.33780070978 13.0095 12.4107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211859_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211859_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:01:54.87 +57:06:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211933_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 211933_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:49:44.85 +51:18:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.168 2169996324686049152 312.43778784217 +51.31102944077 12.9736 12.1295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212110_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212110_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:13:50.09 +52:43:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212152_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212152_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:11:30.15 +53:44:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212301_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212301_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:44:17.00 +55:46:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212340_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212340_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:55:26.36 +56:40:21.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 212491_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212491_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:54:57.21 +57:19:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212583_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212583_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:44:12.53 +55:24:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212694_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212694_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:20.66 +50:21:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212983_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 212983_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:01:40.28 +57:45:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213030_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213030_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:17:49.89 +52:29:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:43:57.18 +56:02:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.194 2184110102608333696 310.98913403817 +56.04429283035 11.9889 10.6247 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213236_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213236_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:18:56.09 +50:04:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213367_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213367_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:46:17.65 +53:01:15.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213431_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213431_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:11:18.82 +57:38:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213434_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213434_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:30:40.42 +57:12:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213446_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213446_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:29:02.08 +55:26:10.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213578_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213578_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:10.05 +54:10:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213597_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213597_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:50:52.33 +55:02:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.317 2183062817785096832 312.71799601210 +55.03478163404 12.8183 12.0849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213636_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213636_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:19:34.82 +53:02:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.616 2175447119213430528 319.89485682314 +53.03882221248 11.8645 10.5067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213660_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213660_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:30:27.51 +52:56:38.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213685_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213685_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:39:57.34 +53:21:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.527 2183157199685211904 309.98962479234 +53.35606368173 13.0429 12.4314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213832_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213832_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:37:09.54 +51:04:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213971_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 213971_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:09:17.88 +53:37:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.538 2176426333096129920 317.32633851397 +53.62941052606 12.6310 11.4705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214084_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214084_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:31:34.91 +52:34:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.869 2181566309449452032 307.89572882464 +52.57261308837 12.9511 11.6448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214191_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214191_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:20:13.61 +56:31:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214210_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214210_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:37:46.39 +53:50:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.113 2183232589257374720 309.44453291754 +53.84551542874 13.3455 12.8120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214246_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214246_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:49:27.62 +56:31:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.039 2189952220206196864 312.36306519782 +56.52149989974 13.3757 12.6675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214259_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214259_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:49:34.94 +50:45:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214267_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214267_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:20.29 +51:20:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214364_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214364_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:46:27.84 +56:54:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214393_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214393_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:33:09.66 +54:22:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.274 2174477556124356224 323.29069379456 +54.38152076901 11.2318 9.6896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214420_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214420_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:46:36.15 +54:55:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.263 2183723177599938176 311.65080143573 +54.91803704394 13.3345 12.8102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214494_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 214494_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214634_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214634_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:52:42.47 +57:11:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.510 2190010150725881216 313.17624354339 +57.19907975148 12.9694 11.9584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214636_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 214636_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214665_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214665_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:03:54.83 +55:27:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214693_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214693_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:29:52.54 +57:48:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214765_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214765_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:36:53.21 +51:07:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.422 2180640043919319936 309.22183062412 +51.12950314505 13.2732 12.5483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214876_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214876_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:35:37.56 +55:22:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.774 2183666449673494784 308.90585273872 +55.37101739163 13.5411 12.9998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214970_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 214970_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:50:10.13 +56:47:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215025_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215025_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:13:23.68 +58:02:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215091_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215091_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:29.43 +54:57:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215096_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215096_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:16:13.35 +56:25:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 2.816 2177379407824832128 319.05614103662 +56.42506154712 13.0666 12.2597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215175_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215175_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:56:54.30 +55:53:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.142 2189088863058865536 314.22729649436 +55.88440188775 13.1534 12.1031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215263_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215263_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:47:49.77 +50:55:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.187 2169961312111879424 311.95693794770 +50.92557025386 13.0630 12.4787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215269_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215269_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:42:45.57 +57:01:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215282_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215282_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:26.18 +54:26:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.143 2183320825064327424 310.60918523533 +54.44867306359 13.0720 12.2605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215456_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215456_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:49:00.29 +54:14:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.888 2182872086881014656 312.25033676222 +54.23643008518 13.4815 12.8792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215457_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215457_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:46:28.18 +54:52:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.061 2183723005801250688 311.61741095869 +54.87509992741 13.1213 12.5032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215620_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215620_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:58:24.03 +55:39:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215701_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215701_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:40:13.76 +53:57:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215741_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215741_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:56:04.95 +51:04:39.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 215745_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215745_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:41.27 +57:26:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.859 2187252094523813632 310.67228799168 +57.44165955595 13.5015 12.8380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215881_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215881_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:59:13.14 +57:18:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.428 2190061003136777728 314.80513546794 +57.30964326370 12.3218 10.9545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215896_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215896_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:16:21.64 +56:24:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.329 2177378686270295296 319.09160097801 +56.41133595689 12.9114 11.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215998_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 215998_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:27:07.33 +55:34:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.302 2177798802795142784 321.78055484361 +55.57158286282 12.5566 11.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 216197_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216197_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:18:44.81 +52:28:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216204_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216204_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:11:20.45 +54:26:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216226_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216226_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:54:45.20 +57:39:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.142 2190139686938608128 313.68892033156 +57.66206663109 13.3204 12.6559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 216268_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216268_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:33:27.57 +56:16:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216478_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216478_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:10:04.73 +53:33:01.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 216519_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216519_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:30:08.18 +54:07:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.399 2181987357978579968 307.53469406930 +54.12242330967 13.4097 12.6039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 216647_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216647_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:03.24 +55:17:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.978 2186562112320102016 308.01285205059 +55.29210145819 13.2621 12.3850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 216927_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 216927_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:19:48.48 +57:30:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217101_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217101_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:38:08.94 +54:56:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.457 2183594947056505216 309.53769494964 +54.94873042422 13.7903 13.2190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 217206_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217206_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:46:01.03 +55:16:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.335 2183749325360985856 311.50504630224 +55.27306982515 13.6754 12.7670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 217370_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217370_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:01:37.73 +57:45:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.506 2190449714856632832 315.40671447571 +57.76299160141 13.3209 12.5547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 217381_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217381_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:59:40.07 +55:32:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217405_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217405_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:55:47.61 +58:15:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217977_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 217977_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:52:14.42 +54:49:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.580 2183006880129978752 313.05976276856 +54.81962954270 13.3978 12.3215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 218243_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 218243_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:47:46.13 +53:19:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.495 2182453825785653376 311.94234773007 +53.33343457037 13.4669 12.7621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 218398_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 218398_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:29:59.64 +52:57:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218567_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 218567_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:48:10.04 +55:50:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218653_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 218653_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:34:51.60 +51:24:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.630 2171722076905263488 323.71475719407 +51.40355482120 12.8548 11.8703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 218982_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 218982_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:48:08.87 +55:51:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.847 2183905662166849408 312.03711584479 +55.85360703630 13.4889 12.8789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219038_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 219038_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:43:06.62 +52:20:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219152_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 219152_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:46:15.93 +53:19:21.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 171293_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 171293_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 135032_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 135032_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:34:23.69 +50:03:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 74759_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:32:45.02 +54:17:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43258_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 43258_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:48:24.39 +55:22:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65541_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 65541_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 62299_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 62299_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 24584_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:42:03.45 +56:54:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22191_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 22191_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:54:14.32 +56:45:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106674_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 106674_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:28:03.66 +52:13:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 23867_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:24:40.25 +57:18:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 57750_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:35:55.07 +54:49:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 103722_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:23:29.62 +52:31:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96626_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 96626_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:46:27.43 +52:18:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91365_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 91365_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:07:18.89 +53:24:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149082_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 149082_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:15:30.48 +51:07:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 134613_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:13:05.28 +50:25:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78940_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 78940_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:38:53.16 +53:29:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96299_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 96299_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 64691_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 64691_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:51:26.74 +53:56:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106095_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 106095_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:34:16.69 +52:08:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93759_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 93759_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:42:10.72 +53:19:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120757_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 120757_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 143451_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 143451_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 173161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 173161_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 28738_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 28738_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 94836_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 94836_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 20:44:44.99 +53:16:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192818_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 192818_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:32:55.75 +51:18:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.012 2171641228438818944 323.23329010553 +51.30202616633 11.2472 9.5566 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 174556_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:01:06.54 +50:07:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192679_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 192679_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:18:21.91 +49:57:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106669_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 106669_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 125047_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:04:54.74 +51:34:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 67289_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:47:52.56 +53:54:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15507_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 15507_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 51830_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 51830_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 138496_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 138496_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 22744_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:26:54.27 +57:22:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85081_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 85081_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 93239_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 93239_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 46334_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 46334_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks
**** FOUND 21:34:09.41 +55:35:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177980_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
Preparing report for the candidate 177980_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
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Considering the candidate 69242_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318
The candidate 69242_fd_Cyg-02-Q2b1x1_2026-03-29_03-41-57_20.00sec_-15.00C_LIGHT_0318 did not pass the final checks