This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2085273318766532096,2461126.9156,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2085273318766532096 20260327.4156 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:41.24 +45:51:48.1 ;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-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4156 2461126.9156 13.07 19:52:53.74 +46:55:28.4
80.97914 9.90571 galactic Cyg Second-epoch detections are separated by 6.1" and 55.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.2153+46.9332 | 19:52:51.68 +46:55:59.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.2153+46.9332,2461126.9156,13.07,0.05,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
ATO J298.2153+46.9332 20260327.4156 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:53.74 +46:55:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4156 2461126.9156 13.38 20:07:50.64 +45:01:34.3
80.67429 6.70350 galactic Cyg Second-epoch detections are separated by 3.2" and 55.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J301.9511+45.0218 | 20:07:50.64 +45:01:34.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6V (Sr) 2016AJ....151...13G LAMOST J200750.23+450118.7
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 J301.9511+45.0218,2461126.9156,13.38,0.05,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 J301.9511+45.0218 20260327.4156 13.38CV 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:50.64 +45:01:34.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4156 2461126.9156 12.26 20:58:46.33 +47:51:04.4
88.16274 1.32110 galactic Cyg Second-epoch detections are separated by 0.9" and 49.1 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 J314.6984+47.8508 | 20:58:46.33 +47:51:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6984+47.8508,2461126.9156,12.26,0.05,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 J314.6984+47.8508 20260327.4156 12.26CV 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:58:46.33 +47:51:04.4 ;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-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_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
KIC 6463513,2461126.9156,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KIC 6463513 20260327.4156 12.94CV 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:56.72 +41:53:00.9 ;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-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20_00sec_-15_00C_LIGHT_0415_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: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
First image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Last image: 2461126.93720301 27.03.2026 10:29:24.340 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
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: 8 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): 24828
Objects passed selection criteria: 24769
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 20358.8
Average stars matched: 18974.8 (93.2019 %)
Memory usage VmPeak: 127628 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:06:02 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: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
First image: 2461036.54266910 27.12.2025 01:01:16.610 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Last image: 2461126.93720301 27.03.2026 10:29:24.340 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 58
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.71
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: 75 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): 166120
Objects passed selection criteria: 165676
Measurements per detected object (mean, median, min, max): 2.8 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 3.0 2 4
Average stars detected per image: 126969
Average stars matched: 118638 (93.4386 %)
Memory usage VmPeak: 2122064 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:09:10 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat to cache
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.89405067
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits exists and is non-empty
Saving wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits to local_wcs_cache/
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits exists and is non-empty
Saving wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits to local_wcs_cache/
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
Saving wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits'
wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits exists and is non-empty
Saving wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:54.520 +45:58:43.65
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:30.634 +46:01:58.33
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 20:23:54.520 +45:58:43.65
Second-epoch second image center 20:23:30.634 +46:01:58.33
Angular distance between the image centers 0.08777 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits &> /tmp/tmp.j72CqJqd3n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits &> /tmp/tmp.7wop9Hyw4f
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.TsNTf0DwwE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits &> /tmp/tmp.wAoWU3Ng4H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
The reference image (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits) and catalog (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat) found
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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 16730 out of 27960 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914223
a=0.000000 b=1.000000 c=22.914223
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
2.4 pix Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
5.1 pix fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
3.5 pix fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Limiting magnitude estimates:
14.9 mag. Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
14.9 mag. Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
13.8 mag. fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
14.4 mag. fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.5 (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.j72CqJqd3n (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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3305, passed=27960
Got 27960 stars (including 24617 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 27960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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.7wop9Hyw4f (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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3383, passed=28049
Got 28049 stars (including 24641 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 28049 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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.TsNTf0DwwE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=773, passed=15696
Got 15696 stars (including 14922 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 15696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.84"
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.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.wAoWU3Ng4H (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1774, passed=24043
Got 24043 stars (including 22256 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat
util/solve_plate_with_UCAC5 got 24043 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
Saving fully-calibrated image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits'
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits'
Preparing the HTML report for the field Cyg-03-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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32565_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 32565_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:05:44.43 +48:32:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32887_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 32887_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:20:25.14 +49:42:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02796_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 02796_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:01:22.08 +50:06:16.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22617_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 22617_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:45:13.97 +42:20:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07414_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 07414_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:58:27.61 +47:38:46.7 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-03-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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat to cache
SExtractor catalog cache: saved Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Creating symlink local_wcs_cache/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits exists and is non-empty
wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits exists and is non-empty
wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:54.520 +45:58:43.65
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:24:01.185 +45:59:58.10
Second-epoch image center 20:23:30.634 +46:01:58.33
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 20:23:54.520 +45:58:43.65
Second-epoch second image center 20:23:30.634 +46:01:58.33
Angular distance between the image centers 0.08777 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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits &> /tmp/tmp.x3WR8r1YfP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits &> /tmp/tmp.FDATrQJbmX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.XHW98P4pC1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits &> /tmp/tmp.aPsKf0J0dY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
Found non-empty wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits and wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
The reference image (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits) and catalog (wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat) found
'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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 18412 out of 199760 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.735380
a=0.000000 b=1.000000 c=22.735380
From vast_summary.log: estimated ref. image limiting mag.: -7.71
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
2.2 pix Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
5.2 pix fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
3.6 pix fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Limiting magnitude estimates:
15.0 mag. Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
15.0 mag. Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
13.9 mag. fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
14.5 mag. fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.2 (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.x3WR8r1YfP (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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=32550, passed=199702
Got 199702 stars (including 166829 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat
util/solve_plate_with_UCAC5 got 199702 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.53"
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 944 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 - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.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.FDATrQJbmX (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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits' -> 'wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Checking if the catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat corresponding to the image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
WCS catalog name: wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=32762, passed=199652
Got 199652 stars (including 166589 good ones) from the SExtractor catalog wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat
util/solve_plate_with_UCAC5 got 199652 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits -region wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.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.XHW98P4pC1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=8538, passed=70008
Got 70008 stars (including 61439 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 70008 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 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: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.84"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 924 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.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.aPsKf0J0dY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Checking if the catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat corresponding to the image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
WCS catalog name: wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=18141, passed=116711
Got 116711 stars (including 98478 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat
util/solve_plate_with_UCAC5 got 116711 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 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: 0.70"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits -region wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.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-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits
Saving fully-calibrated image wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_Cyg-03-Q2b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_04-27-15_20.00sec_-15.00C_LIGHT_0415.fits
Saving fully-calibrated image wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-03-Q2b1x1_070339_TTUQ2b1x1_1074_cjerSMP8/wcs_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484.fits
Preparing the HTML report for the field Cyg-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out108461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out225598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out133458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out225530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out225573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53128.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 3s
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Considering the candidate 225530_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
Preparing report for the candidate 225530_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
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Considering the candidate 225538_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225538_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:41:58.07 +43:56:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.764 2069998039933670912 310.49051741255 +43.93895446818 12.8730 12.3915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225540_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225540_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 19:49:57.63 +43:19:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.066 2078737684211240448 297.48982081292 +43.33158117945 13.1297 12.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225550_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225550_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:22:49.02 +49:24:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.560 2084769501922351360 305.70524669168 +49.40780212146 12.6899 11.8259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225556_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225556_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:56:04.91 +45:31:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.349 2163126193772639872 314.01967543600 +45.52944573713 12.7019 12.2511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225565_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225565_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:22:13.64 +49:48:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.448 2084831727410014976 305.55759377589 +49.81674876757 13.1530 12.4121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225567_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225567_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:57:22.40 +46:29:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.154 2163752400007902592 314.34300944603 +46.48479742082 12.4692 11.6198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225568_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225568_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:21:36.44 +47:46:44.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 225573_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
Preparing report for the candidate 225573_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
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Considering the candidate 225586_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225586_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:31:26.43 +45:26:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.038 2070800206691947136 307.85976771176 +45.43800767199 12.7802 12.3325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 225596_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225596_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:06:07.12 +49:36:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225598_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 225598_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:49:18.96 +48:16:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.466 2167163226821823616 312.33035204501 +48.27522925519 13.2485 12.5930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 229844_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 229844_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:45:07.97 +45:44:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230322_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 230322_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:30:03.05 +45:54:01.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 232281_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 232281_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:47:53.29 +47:51:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 233056_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 233056_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:05:41.36 +47:45:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233063_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 233063_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:25:41.95 +41:52:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233080_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 233080_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:45:34.19 +46:13:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233401_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 233401_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:49:02.44 +46:09:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233627_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 233627_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:26:12.21 +45:23:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234138_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 234138_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 19:59:12.11 +48:43:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235664_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 235664_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:14:27.77 +47:29:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235938_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 235938_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:42:28.82 +45:48:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236045_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 236045_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 92833_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 92833_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:19:08.48 +46:53:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133458_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
Preparing report for the candidate 133458_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
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Considering the candidate 54267_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 54267_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:05:44.38 +48:32:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108461_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 108461_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:57:23.74 +45:31:45.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 49127_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 49127_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:54:36.87 +48:10:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53128_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
Preparing report for the candidate 53128_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
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Considering the candidate 169535_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
Preparing report for the candidate 169535_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
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Considering the candidate 140134_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 140134_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:13:40.65 +44:37:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181251_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 181251_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:45:13.92 +42:20:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58402_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 58402_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:58:27.63 +47:38:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22483_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 22483_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:57:14.30 +49:27:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30523_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 30523_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:20:25.13 +49:42:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124593_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 124593_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:16:00.96 +45:34:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 36727_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 36727_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:27:02.67 +49:23:03.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 63139_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 63139_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 20:04:28.96 +48:13:48.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68302_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 68302_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 19:52:07.40 +47:55:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 92070_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 92070_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks
**** FOUND 19:51:59.24 +47:01:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31326_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484
The candidate 31326_fd_Cyg-03-Q2b1x1_2026-03-27_05-29-24_20.00sec_-14.90C_LIGHT_0484 did not pass the final checks