This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 13.15 21:25:48.95 +47:36:05.8
91.10341 -2.15565 galactic Cyg Second-epoch detections are separated by 3.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.4564+47.5993 | 21:25:48.95 +47:36:05.8 (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 J321.4564+47.5993,2461126.9067,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.4564+47.5993 20260327.4067 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:48.95 +47:36:05.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J211356.75+472623.0,2461126.9067,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J211356.75+472623.0 20260327.4067 13.10CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:57.66 +47:26:04.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.88 21:30:04.49 +47:49:06.6
91.77172 -2.49391 galactic Cyg Second-epoch detections are separated by 7.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.5305+47.8239 | 21:30:04.49 +47:49:06.6 (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 J322.5305+47.8239,2461126.9067,12.88,0.05,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 J322.5305+47.8239 20260327.4067 12.88CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:04.49 +47:49:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9067,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4067 12.66CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:42.35 +41:49:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9067,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4067 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:55.62 +48:31:30.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.65 21:31:29.89 +49:00:41.2
92.76055 -1.78506 galactic Cyg Second-epoch detections are separated by 7.2" and 1.6 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 J322.8708+49.0038 | 21:31:29.89 +49:00:41.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.8708+49.0038,2461126.9067,12.65,0.05,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 J322.8708+49.0038 20260327.4067 12.65CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:31:29.89 +49:00:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5840473,2461126.9067,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5840473 20260327.4067 12.70CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:02:14.78 +47:06:36.3 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.34 22:12:29.04 +48:44:28.2
97.83890 -6.23106 galactic Lac Second-epoch detections are separated by 3.6" and 3.2 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 J333.1202+48.7381 | 22:12:31.36 +48:43:56.0 (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 J333.1202+48.7381,2461126.9067,12.34,0.05,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 J333.1202+48.7381 20260327.4067 12.34CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:29.04 +48:44:28.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.06 21:57:06.93 +49:00:53.9
95.96098 -4.50974 galactic Cyg Second-epoch detections are separated by 7.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2849+49.0139 | 21:57:06.11 +49:01:16.0 (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 J329.2849+49.0139,2461126.9067,12.06,0.05,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 J329.2849+49.0139 20260327.4067 12.06CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:06.93 +49:00:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2164528762609901440,2461126.9067,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2164528762609901440 20260327.4067 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:12:06.28 +47:46:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_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
V2599 Cyg,2461126.9067,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2599 Cyg 20260327.4067 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:08.00 +42:29:35.9 ;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-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_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
V0631 Cyg,2461126.9067,12.06,0.05,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
V0631 Cyg 20260327.4067 12.06CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:09.07 +43:51:34.3 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 11.26 21:33:24.66 +48:29:25.8
92.63767 -2.38147 galactic Cyg Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1978640447732492032 | 21:33:24.76 +48:29:34.8 (Gaia DR3) | T | P | 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
Gaia DR3 1978640447732492032,2461126.9067,11.26,0.05,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
Gaia DR3 1978640447732492032 20260327.4067 11.26CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:33:24.66 +48:29:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.52 21:27:52.38 +43:27:03.1
88.47299 -5.39155 galactic Cyg Second-epoch detections are separated by 3.1" and 3.2 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 | target | 21:27:52.38 +43:27:03.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9067,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4067 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:52.38 +43:27:03.1 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4067 2461126.9067 12.71 21:30:05.76 +44:18:19.4
89.35657 -5.05032 galactic Cyg Second-epoch detections are separated by 1.6" and 3.2 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 J322.5369+44.3059 | 21:30:05.76 +44:18:19.4 (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 J322.5369+44.3059,2461126.9067,12.71,0.05,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 J322.5369+44.3059 20260327.4067 12.71CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:05.76 +44:18:19.4 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973611865649234560,2461126.9067,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973611865649234560 20260327.4067 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:56.08 +45:48:33.4 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9067,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4067 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:37.48 +45:57:31.9 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1975887682925279360,2461126.9067,12.49,0.05,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 1975887682925279360 20260327.4067 12.49CV 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:10:14.98 +48:44:00.4 ;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-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20_00sec_-15_00C_LIGHT_0438_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20_00sec_-15_00C_LIGHT_0437_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: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461126.90702715 27.03.2026 09:45:57.146 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 26786
Objects passed selection criteria: 26662
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 19545.8
Average stars matched: 18520.2 (94.7533 %)
Memory usage VmPeak: 130180 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 07:10:50 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: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461036.55649360 27.12.2025 01:21:11.047 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461126.90702715 27.03.2026 09:45:57.146 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 195
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 49 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): 192582
Objects passed selection criteria: 192060
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 134972
Average stars matched: 127341 (94.346 %)
Memory usage VmPeak: 1950900 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 07:15:49 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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: 2461126.90647143
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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
Saving wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits to local_wcs_cache/
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits'
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits exists and is non-empty
Saving wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:48.997 +45:57:04.52
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:50.452 +45:57:14.47
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:35:48.997 +45:57:04.52
Second-epoch second image center 21:35:50.452 +45:57:14.47
Angular distance between the image centers 0.00504 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.34Rjh5STdG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.aG5HpDUwIt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits &> /tmp/tmp.JrnGPLMveq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits &> /tmp/tmp.pVbyfAOEHc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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 14243 out of 30795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.935356
a=0.000000 b=1.000000 c=22.935356
From vast_summary.log: estimated ref. image limiting mag.: -8.07
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 14 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.4 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
4.2 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
4.7 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Limiting magnitude estimates:
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
14.9 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
13.7 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
13.6 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.34Rjh5STdG (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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3934, passed=30795
Got 30795 stars (including 26843 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 30795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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.aG5HpDUwIt (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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3890, passed=30626
Got 30626 stars (including 26706 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 30626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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.JrnGPLMveq (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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=724, passed=14243
Got 14243 stars (including 13515 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat
util/solve_plate_with_UCAC5 got 14243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 1.05"
Excluding outliers - 933 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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.pVbyfAOEHc (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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=643, passed=13226
Got 13226 stars (including 12580 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat
util/solve_plate_with_UCAC5 got 13226 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.94"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.95"
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 935 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-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits'
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 53042_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 53042_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:48:31.53 +42:05:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22924_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 22924_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:04:56.66 +43:55:43.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11124_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 11124_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:06:36.88 +47:38:52.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05487_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 05487_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:46:47.72 +49:18:35.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18803_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 18803_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:36:02.60 +45:22:28.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18301_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 18301_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:58.76 +45:35:28.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 12359_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:08:45.11 +47:24:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04384_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 04384_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:48.57 +49:49:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16550_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 16550_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:58:24.44 +45:52:21.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17410_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 17410_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:42:08.39 +45:45:56.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15195_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 15195_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:29:27.24 +46:32:29.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24427_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 24427_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:11.28 +43:16:29.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23153_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 23153_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:18:27.37 +43:56:46.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18402_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 18402_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:06:01.65 +45:00:51.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cyg-04-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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Creating symlink local_wcs_cache/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits exists and is non-empty
wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:48.997 +45:57:04.52
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:35:59.427 +46:00:14.09
Second-epoch image center 21:35:50.452 +45:57:14.47
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:35:48.997 +45:57:04.52
Second-epoch second image center 21:35:50.452 +45:57:14.47
Angular distance between the image centers 0.00504 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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.n88GyK0KBu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.vr0W0GmrOU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits &> /tmp/tmp.H6NIR9nY89
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits &> /tmp/tmp.9p93BIgvBF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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 15408 out of 227547 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.745984
a=0.000000 b=1.000000 c=22.745984
From vast_summary.log: estimated ref. image limiting mag.: -7.72
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 145 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
2.2 pix Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
4.2 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
4.8 pix fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Limiting magnitude estimates:
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
15.0 mag. Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
13.8 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
13.7 mag. fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 12.9 (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.n88GyK0KBu (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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=44928, passed=227506
Got 227506 stars (including 182305 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 227506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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.vr0W0GmrOU (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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=45138, passed=228742
Got 228742 stars (including 183314 good ones) from the SExtractor catalog wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 228742 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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.H6NIR9nY89 (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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=9160, passed=77300
Got 77300 stars (including 68103 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat
util/solve_plate_with_UCAC5 got 77300 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 935 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-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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.9p93BIgvBF (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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Checking if the catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat corresponding to the image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
WCS catalog name: wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=8274, passed=68424
Got 68424 stars (including 60112 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat
util/solve_plate_with_UCAC5 got 68424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 931 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cyg-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits -region wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits
Saving fully-calibrated image wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-50_20.00sec_-15.00C_LIGHT_0023.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-09_20.00sec_-15.00C_LIGHT_0437.fits
Saving fully-calibrated image wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.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-04-Q2b1x1_070540_TTUQ2b1x1_10481_dd4aCUmq/wcs_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438.fits
Preparing the HTML report for the field Cyg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out106928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out240030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out98677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out265225.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out108279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61603.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 34s
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: 11s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257938_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257938_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:58:20.02 +43:23:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.180 1960989025483205504 329.58287666248 +43.39893330002 12.8252 12.2369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257946_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257946_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257948_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257948_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257957_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257957_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:59:15.54 +46:49:23.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257962_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257962_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257964_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257964_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257966_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257966_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257968_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257968_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:21.64 +48:19:55.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257969_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257969_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257971_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257971_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:12:34.52 +42:09:11.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257974_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257974_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:47:12.79 +49:49:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257990_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257990_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257992_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 257992_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:06:35.26 +47:21:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257993_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257993_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257994_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257994_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257998_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 257998_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 258004_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:51:36.26 +49:16:40.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258005_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 258005_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258007_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 258007_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261573_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 261573_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:05:53.60 +48:16:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261598_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 261598_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:41:51.54 +45:45:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261680_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 261680_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:08:20.03 +49:14:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261703_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 261703_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261856_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 261856_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:15:43.95 +47:57:24.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262381_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 262381_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262684_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 262684_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262799_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 262799_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:35:51.05 +45:24:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263072_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263072_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:56:53.31 +48:40:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263298_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263298_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:03:42.76 +49:44:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263675_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263675_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:41:48.57 +45:45:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263816_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263816_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263818_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263818_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:29.41 +45:51:17.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263999_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 263999_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:39:14.56 +46:09:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264118_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264118_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:51:52.36 +41:38:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264185_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264185_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:11:00.55 +49:04:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264193_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264193_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264244_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264244_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:07:58.18 +44:11:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264273_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264273_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:28:12.71 +45:46:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.819 1971400129302130688 322.05403889597 +45.77578273896 12.8671 12.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264501_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264501_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:55:46.96 +49:50:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264801_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264801_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:22:49.36 +46:30:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264930_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 264930_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:49:09.67 +49:42:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265037_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265037_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265087_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265087_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:29:35.87 +46:24:13.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265225_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265225_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:05:13.25 +49:19:44.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265331_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265331_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:51:21.64 +44:39:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265369_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265369_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:29:03.58 +47:16:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265424_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265424_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:53:25.78 +42:43:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265638_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265638_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265674_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265674_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265847_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265847_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265933_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265933_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:22:56.27 +45:29:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265974_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 265974_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266089_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266089_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:37:37.77 +46:00:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266138_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266138_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266202_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266202_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:52:39.97 +47:06:00.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266216_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266216_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266218_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266218_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266393_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266393_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:51:50.05 +46:11:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266622_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266622_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:42:41.64 +43:34:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266771_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266771_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266779_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266779_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266908_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 266908_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267028_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267028_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267102_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267102_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267246_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267246_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267249_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267249_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:57:44.83 +45:54:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267298_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267298_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267299_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267299_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267415_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267415_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267444_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267444_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267450_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267450_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267492_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267492_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267493_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267493_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267528_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267528_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267578_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 267578_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86476_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 86476_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:06:36.84 +47:38:52.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175379_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 175379_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:04:56.67 +43:55:43.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42539_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 42539_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:46:47.73 +49:18:35.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161501_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 161501_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:13.59 +44:27:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138802_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 138802_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:58.89 +45:35:28.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146074_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 146074_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:36:02.98 +45:22:28.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137859_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 137859_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:13.03 +45:27:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240192_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 240192_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61617_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 61617_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:39:39.32 +48:26:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87004_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 87004_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:38:24.94 +47:22:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87861_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 87861_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:16:09.92 +47:29:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172772_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 172772_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192707_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 192707_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:20:23.80 +43:18:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86368_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 86368_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:43:56.13 +47:21:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85272_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 85272_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:32.39 +47:26:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 130655_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:38:32.12 +45:42:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169996_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 169996_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:41:01.74 +43:56:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217051_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 217051_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:18:58.00 +41:53:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61603_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 61603_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149014_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 149014_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:34:09.20 +44:59:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 153896_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:45:01.50 +44:39:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 171889_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:37:14.83 +43:52:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58347_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 58347_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:47:07.53 +48:28:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127915_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 127915_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:29:19.79 +45:56:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 89637_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:08:45.10 +47:24:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255695_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 255695_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:22:09.03 +43:32:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83186_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 83186_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:07:38.30 +47:00:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246477_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 246477_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 216586_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:11:37.24 +41:51:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 57451_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:10:10.26 +48:42:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120491_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 120491_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:58:24.39 +45:52:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73683_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 73683_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:45:04.21 +47:54:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150267_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 150267_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:01:42.99 +44:55:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31202_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 31202_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:48.58 +49:49:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196331_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 196331_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106928_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 106928_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:43:19.70 +46:33:26.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98677_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 98677_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:11:31.74 +47:00:35.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28736_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 28736_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182078_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 182078_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:15:33.19 +42:41:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 178552_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:39:17.18 +42:26:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164484_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 164484_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94270_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 94270_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:10:57.47 +46:27:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121466_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 121466_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:09:04.89 +45:30:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76275_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 76275_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:09:38.83 +47:15:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240030_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 240030_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:07:26.24 +49:31:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.355 1976734306881110400 331.85816002684 +49.52229615907 12.6298 11.8469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122229_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 122229_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 224886_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:48:31.51 +42:05:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35847_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 35847_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:00:09.59 +49:13:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108279_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 108279_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40538_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
Preparing report for the candidate 40538_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131667_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 131667_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:33:18.13 +45:51:14.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134409_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 134409_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:42:08.40 +45:45:55.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157414_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 157414_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:37:27.81 +44:41:47.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115357_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 115357_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:29:27.28 +46:32:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110364_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 110364_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:25:20.16 +46:42:53.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 134934_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:35:38.63 +45:34:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189554_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 189554_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:40:11.29 +43:16:29.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36682_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 36682_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:42:38.92 +49:36:01.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57487_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 57487_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:26:51.97 +48:50:07.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174503_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 174503_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:18:27.38 +43:56:47.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30344_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 30344_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:32:56.68 +49:58:40.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43891_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 43891_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:22:00.68 +49:23:19.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180991_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 180991_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:17:23.21 +42:41:01.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42320_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 42320_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:19:28.77 +49:30:36.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223368_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 223368_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:16:29.65 +42:15:07.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148743_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 148743_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:02:56.52 +44:39:00.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96108_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 96108_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:05:16.03 +46:44:42.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139317_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 139317_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 22:06:01.68 +45:00:51.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157310_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 157310_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks
**** FOUND 21:02:24.49 +44:47:28.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122710_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438
The candidate 122710_fd_Cyg-04-Q2b1x1_2026-03-27_04-45-57_20.00sec_-15.00C_LIGHT_0438 did not pass the final checks