This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.9139,14.46,0.05,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 20260321.4139 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:43:14.19 +50:43:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.37 20:35:30.11 +52:07:55.8
89.17428 6.91186 galactic Cyg Second-epoch detections are separated by 5.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:35:30.11 +52:07:55.8 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.049 (G)
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,2461120.9139,14.37,0.05,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 20260321.4139 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:30.11 +52:07:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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 2182753889379575168,2461120.9139,14.39,0.05,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 2182753889379575168 20260321.4139 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:27.49 +54:18:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.32 20:42:18.85 +52:16:49.3
89.92502 6.16695 galactic Cyg Second-epoch detections are separated by 1.0" and 4.2 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 | DocumentRef: VOTx3434890 | 20:42:18.85 +52:16:49.3 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.366+/-0.038 (G)
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
DocumentRef: VOTx3434890,2461120.9139,14.32,0.05,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
DocumentRef: VOTx3434890 20260321.4139 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:42:18.85 +52:16:49.3 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.50 20:43:08.95 +55:29:08.3
92.56269 8.02124 galactic Cep Second-epoch detections are separated by 1.6" and 4.5 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 | 20:43:08.95 +55:29:08.3 (user input) | T | P | (position from user input) J-Ks=1.231+/-0.028 (M)
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,2461120.9139,14.50,0.05,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 20260321.4139 14.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:43:08.95 +55:29:08.3 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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
WISE J205454.4+563538,2461120.9139,14.27,0.05,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
WISE J205454.4+563538 20260321.4139 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:54:56.77 +56:35:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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,2461120.9139,14.05,0.05,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 20260321.4139 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:06.57 +54:38:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.11 21:34:53.09 +51:05:34.3
94.57101 -0.62253 galactic Cyg Second-epoch detections are separated by 5.8" and 5.4 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 J323.7243+51.0915 | 21:34:53.09 +51:05:34.3 (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 J323.7243+51.0915,2461120.9139,14.11,0.05,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 J323.7243+51.0915 20260321.4139 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:53.09 +51:05:34.3 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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,2461120.9139,13.88,0.05,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
target 20260321.4139 13.88CV 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-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:35.57 +55:09:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.89 20:35:10.94 +53:32:42.7
90.29490 7.78580 galactic Cyg Second-epoch detections are separated by 1.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3441899 | 20:35:10.94 +53:32:42.7 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.576+/-0.043 (K)
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
DocumentRef: VOTx3441899,2461120.9139,13.89,0.05,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
DocumentRef: VOTx3441899 20260321.4139 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:10.94 +53:32:42.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.74 20:28:40.48 +55:01:23.2
90.95649 9.41613 galactic Cyg Second-epoch detections are separated by 2.2" and 4.3 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 J307.1582+55.0244 | 20:28:40.48 +55:01:23.2 (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 J307.1582+55.0244,2461120.9139,13.74,0.05,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 J307.1582+55.0244 20260321.4139 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:40.48 +55:01:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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 1979286204650287104,2461120.9139,13.87,0.05,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 1979286204650287104 20260321.4139 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:05.59 +50:31:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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 J214535.17+520917.0,2461120.9139,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214535.17+520917.0 20260321.4139 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:36.07 +52:09:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.32 20:33:37.60 +52:36:19.9
89.38955 7.42214 galactic Cyg Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:33:37.60 +52:36:19.9 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.039 (F)
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,2461120.9139,13.32,0.05,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 20260321.4139 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:33:37.60 +52:36:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213752.77+510405.8,2461120.9139,12.70,0.05,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
ASASSN-V J213752.77+510405.8 20260321.4139 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-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:37:52.75 +51:04:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.29 20:42:40.24 +51:01:42.1
88.96294 5.35806 galactic Cyg Second-epoch detections are separated by 0.9" and 4.2 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 | Gaia DR3 2180477277532374016 | 20:42:37.43 +51:02:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.460+/-0.032 (G)
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 2180477277532374016,2461120.9139,13.29,0.05,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 2180477277532374016 20260321.4139 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:42:40.24 +51:01:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.49 21:48:19.07 +53:05:55.7
97.44357 -0.46114 galactic Cyg Second-epoch detections are separated by 1.2" and 4.4 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 J327.0892+53.1080 | 21:48:19.07 +53:05:55.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.0892+53.1080,2461120.9139,13.49,0.05,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
ATO J327.0892+53.1080 20260321.4139 13.49CV 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-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:19.07 +53:05:55.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.38 21:15:32.00 +54:44:03.3
95.02011 4.01946 galactic Cyg Second-epoch detections are separated by 6.1" and 4.6 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 J318.8915+54.7447 | 21:15:32.00 +54:44:03.3 (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 J318.8915+54.7447,2461120.9139,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.8915+54.7447 20260321.4139 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:15:32.00 +54:44:03.3 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 13.64 20:36:53.67 +52:45:04.1
89.80305 7.10862 galactic Cyg Second-epoch detections are separated by 1.2" and 4.3 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 | DocumentRef: VOTx3524048 | 20:36:53.67 +52:45:04.1 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.453+/-0.033 (G)
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
DocumentRef: VOTx3524048,2461120.9139,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3524048 20260321.4139 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:36:53.67 +52:45:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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 2171930640520535808,2461120.9139,13.74,0.05,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 2171930640520535808 20260321.4139 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:04.42 +50:47:53.9 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.10 20:44:31.87 +55:20:08.5
92.56345 7.77435 galactic Cep Second-epoch detections are separated by 2.2" and 4.7 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 J311.1159+55.3396 | 20:44:31.87 +55:20:08.5 (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 J311.1159+55.3396,2461120.9139,14.10,0.05,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
ATO J311.1159+55.3396 20260321.4139 14.10CV 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-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:31.87 +55:20:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.12 20:30:37.90 +50:36:55.4
87.48849 6.63671 galactic Cyg Second-epoch detections are separated by 2.0" and 4.6 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 | DocumentRef: VOTx3570771 | 20:30:37.90 +50:36:55.4 (user input) | (GCVS) | (GCVS) | (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
DocumentRef: VOTx3570771,2461120.9139,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3570771 20260321.4139 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:37.90 +50:36:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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,2461120.9139,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.4139 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:53.97 +57:03:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4139 2461120.9139 14.30 20:53:08.97 +50:43:26.3
89.76245 3.87826 galactic Cyg Second-epoch detections are separated by 3.2" and 3.8 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 J313.2916+50.7247 | 20:53:08.97 +50:43:26.3 (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 J313.2916+50.7247,2461120.9139,14.30,0.05,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 J313.2916+50.7247 20260321.4139 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:53:08.97 +50:43:26.3 ;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-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20_00sec_-15_00C_LIGHT_0432_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: 2461032.58447227 23.12.2025 02:01:28.404 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461032.58447227 23.12.2025 02:01:28.404 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461120.91419586 21.03.2026 09:56:16.522 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 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): 26372
Objects passed selection criteria: 26278
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 21239.5
Average stars matched: 19787 (93.1613 %)
Memory usage VmPeak: 128044 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 05:00:34 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: 2461032.58447227 23.12.2025 02:01:28.404 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461032.58447227 23.12.2025 02:01:28.404 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461120.91419586 21.03.2026 09:56:16.522 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 162
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 109 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): 186909
Objects passed selection criteria: 186456
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 149318
Average stars matched: 138793 (92.9514 %)
Memory usage VmPeak: 1998476 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 05:03:54 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.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: 2461120.91363054
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits'
wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:38.398 +53:59:42.81
Second-epoch image center 21:10:29.661 +53:57:07.41
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:38.398 +53:59:42.81
Second-epoch image center 21:10:30.380 +53:57:32.94
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:29.661 +53:57:07.41
Second-epoch second image center 21:10:30.380 +53:57:32.94
Angular distance between the image centers 0.00731 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.j58GiJRxby
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits &> /tmp/tmp.gqTK60XM2K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits &> /tmp/tmp.SbWXadpCsy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits &> /tmp/tmp.Waylc7VxyA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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 12554 out of 28559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930525
a=0.000000 b=1.000000 c=22.930525
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
2.2 pix Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
2.7 pix fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
2.8 pix fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Limiting magnitude estimates:
15.1 mag. Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
15.1 mag. Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
14.8 mag. fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
14.8 mag. fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.j58GiJRxby (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3553, passed=28559
Got 28559 stars (including 24952 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 28559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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.gqTK60XM2K (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3534, passed=28454
Got 28454 stars (including 24878 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 28454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits -region wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.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.SbWXadpCsy (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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2061, passed=24578
Got 24578 stars (including 22491 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat
util/solve_plate_with_UCAC5 got 24578 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.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.Waylc7VxyA (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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2050, passed=24696
Got 24696 stars (including 22620 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat
util/solve_plate_with_UCAC5 got 24696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34883.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31632_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 31632_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:57:13.44 +53:46:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.103 2182706507299906560 314.30554844449 +53.78240058084 12.1658 11.6834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31635_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 31635_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:14:01.86 +52:22:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31637_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 31637_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:51:47.13 +55:08:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33374_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 33374_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:35:54.86 +54:49:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33978_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 33978_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:32:45.00 +54:17:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34141_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34141_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:44:57.15 +54:25:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34147_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34147_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:44:10.76 +54:06:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34183_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34183_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:12:54.68 +52:45:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34249_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34249_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:47:52.63 +53:54:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34268_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34268_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:54:14.36 +56:45:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34322_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34322_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:44:44.95 +53:16:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34413_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34413_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:12:30.71 +55:38:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34449_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34449_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:19:45.80 +54:58:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34455_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34455_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:49:59.71 +54:15:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34507_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34507_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:45.18 +53:07:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34510_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34510_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:57.74 +50:33:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.505 2171958265751183104 319.74038613625 +50.55661894674 11.9568 11.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34534_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34534_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:42:03.59 +56:54:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34543_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34543_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:19:51.45 +53:17:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34597_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34597_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:07:37.15 +53:32:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.029 2176422798343176448 316.90452963117 +53.53798957509 11.8414 11.2462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34622_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34622_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:37:55.22 +57:23:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34623_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34623_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:55:54.72 +57:02:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.259 2199009481607891072 328.97737763667 +57.04671784818 12.0565 11.5482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34632_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34632_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:05:58.77 +55:29:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34637_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34637_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:31:32.39 +55:04:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.933 2177545326695659776 322.88454322451 +55.08174242270 12.0753 11.5530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34647_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34647_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:13:13.49 +53:39:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34698_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34698_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:38:45.81 +52:36:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34730_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34730_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:16:47.83 +54:11:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34754_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34754_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:05:34.43 +54:04:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.478 2176682901564421120 316.39344488335 +54.07827130947 11.9826 11.5036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34799_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34799_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:23:15.02 +53:54:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34805_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34805_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:28:44.02 +51:08:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.697 2171667994675671552 322.18342152596 +51.13669362675 11.6753 10.7275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34806_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34806_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:13:05.38 +50:25:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.091 2166172360680078592 318.27194187297 +50.42497967715 10.0788 8.4889 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34808_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34808_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:20:19.36 +54:18:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.113 2176138643315101312 320.08030728345 +54.30964375368 11.6078 10.6262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34823_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34823_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:14:19.81 +52:06:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34831_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34831_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:12:20.52 +52:27:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.209 2175555554246659584 318.08540062982 +52.45041373056 12.0182 11.4854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34841_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34841_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:12:27.34 +54:16:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.713 2176559030407763200 318.11362534353 +54.26693460208 11.9320 11.2946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34846_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34846_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:06:46.17 +54:00:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.641 2176491861417657472 316.69226219943 +54.00672094227 11.9439 11.4058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34874_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34874_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:20:58.28 +53:06:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34883_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 34883_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:18.89 +52:01:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.228 2172376148880200064 319.57848539514 +52.02775680822 11.9867 11.4698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits exists and is non-empty
wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:38.398 +53:59:42.81
Second-epoch image center 21:10:29.661 +53:57:07.41
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:38.398 +53:59:42.81
Second-epoch image center 21:10:30.380 +53:57:32.94
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:10:29.661 +53:57:07.41
Second-epoch second image center 21:10:30.380 +53:57:32.94
Angular distance between the image centers 0.00731 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.Sxd2IaFMfI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits &> /tmp/tmp.G1s45O7gAd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits &> /tmp/tmp.djVxhzvp4r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits &> /tmp/tmp.ICzyEXNa13
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
Found non-empty wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
The reference image (wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat) found
'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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 13078 out of 208449 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.766947
a=0.000000 b=1.000000 c=22.766947
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 110 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
2.0 pix Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
2.6 pix fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
2.6 pix fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Limiting magnitude estimates:
15.3 mag. Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
15.2 mag. Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
14.9 mag. fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
14.8 mag. fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Sxd2IaFMfI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=34209, passed=208406
Got 208406 stars (including 173827 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 208406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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.G1s45O7gAd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits' -> 'wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat corresponding to the image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=34105, passed=208445
Got 208445 stars (including 173944 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 208445 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits -region wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.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.djVxhzvp4r (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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=18329, passed=140219
Got 140219 stars (including 121730 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat
util/solve_plate_with_UCAC5 got 140219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.68"
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 967 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: 0.67"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.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.ICzyEXNa13 (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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=18158, passed=138412
Got 138412 stars (including 120098 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat
util/solve_plate_with_UCAC5 got 138412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.66"
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_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits
Saving fully-calibrated image wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-55-27_20.00sec_-15.00C_LIGHT_0432.fits
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.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_2026-03-21_CI_Cyg-02-Q2b1x1_045654_TTUQ2b1x1_11414_Uu1km6MZ/wcs_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433.fits
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out248384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out252216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out255015.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out235315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254527.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 352s
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: 15s
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Considering the candidate 235315_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235315_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235316_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235316_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235318_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235318_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235323_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235323_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235344_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235344_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235349_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235349_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235370_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235370_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235372_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235372_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235385_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235385_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235390_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235390_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235391_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235391_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235393_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235393_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:13:27.79 +57:06:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235394_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235394_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:45:57.22 +55:32:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235397_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235397_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:30:17.17 +51:35:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235401_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235401_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235402_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235402_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235412_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235412_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:42:40.79 +53:16:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235413_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235413_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:22:42.41 +50:30:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235415_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235415_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 235423_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235423_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:34:38.85 +51:07:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235426_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235426_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:33:51.15 +52:18:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235427_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 235427_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:38:30.13 +50:10:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235428_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 235428_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
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Considering the candidate 237779_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 237779_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:39:12.07 +57:29:56.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 238826_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 238826_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:38:51.00 +57:27:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 239535_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 239535_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:37:09.62 +51:04:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240364_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 240364_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:43:18.79 +52:26:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241825_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 241825_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:40:36.92 +54:17:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242655_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 242655_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:36:07.06 +51:40:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242704_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 242704_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:46:05.02 +52:51:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242707_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 242707_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:31:40.81 +55:04:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242746_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 242746_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:43:25.18 +52:25:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242872_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 242872_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:29:59.42 +52:57:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243109_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 243109_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:22:48.47 +54:12:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243591_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 243591_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:37:30.23 +51:04:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243720_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 243720_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:36:08.63 +51:40:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244147_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 244147_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:50:45.16 +55:14:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244211_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 244211_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:35:51.73 +54:41:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244301_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 244301_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:11:37.02 +49:54:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244363_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 244363_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:32:29.92 +54:57:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244522_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 244522_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:21:01.16 +55:24:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244573_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 244573_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244587_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 244587_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244604_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 244604_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245108_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245108_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:07:18.37 +49:46:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245243_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245243_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:33:56.46 +50:46:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245491_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245491_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:49:57.84 +54:16:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245638_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245638_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:03:54.94 +55:27:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245856_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245856_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:32:47.89 +51:13:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245913_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 245913_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:51:30.09 +54:44:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:32:53.29 +51:00:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246111_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246111_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:47:35.87 +55:35:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246331_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246331_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:39:11.83 +54:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246599_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246599_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:38:34.07 +56:58:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246609_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246609_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:41:01.32 +57:09:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246764_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246764_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:13:23.68 +58:02:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246788_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246788_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:27:03.41 +50:03:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246819_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 246819_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246984_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 246984_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:50:43.84 +55:13:09.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 247054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:22:23.50 +55:35:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247453_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 247453_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:43:16.76 +56:27:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247614_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 247614_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:24:09.47 +52:26:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247856_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 247856_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:47:39.16 +55:38:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248093_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248093_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:10.52 +51:16:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248261_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 248261_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248360_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248360_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:40:13.19 +57:30:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248384_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248384_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:40:36.81 +54:16:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.697 2174335100653153024 325.15412254966 +54.27707166348 13.3396 12.3606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248572_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248572_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:31:22.32 +52:13:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248677_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248677_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:45.12 +51:16:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248787_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248787_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:39:07.83 +56:02:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248833_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248833_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:43:00.71 +53:45:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248882_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 248882_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:39:21.80 +51:45:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249033_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 249033_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:54:05.21 +53:46:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249177_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 249177_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:42:02.14 +57:37:24.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249607_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 249607_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:32:13.12 +51:52:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249709_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 249709_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:28:33.77 +56:24:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249796_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 249796_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:23:38.95 +50:02:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.910 2171130470933812480 320.91107812316 +50.04229818596 14.3507 13.6538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250361_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 250361_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:42:46.74 +53:59:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250807_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 250807_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:51:55.12 +55:14:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.275 2174070496302206592 327.97975428782 +55.23858105547 13.9776 13.3535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251003_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251003_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:24:29.71 +56:21:19.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251144_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251144_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:32:51.96 +54:39:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251272_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 251272_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251288_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251288_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:00:41.27 +58:05:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251311_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251311_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:46:58.76 +51:03:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251374_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251374_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:25:52.91 +49:56:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251983_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 251983_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:42:37.58 +56:14:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252000_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252000_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:23:58.79 +53:07:48.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252126_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252126_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:26:32.70 +52:55:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252166_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252166_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:52:37.72 +50:28:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252216_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252216_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:34:15.37 +49:44:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.946 2179977691241388416 308.56366931640 +49.74828298643 14.2806 13.6173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252390_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252390_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:44:11.07 +52:31:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252672_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252672_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:04:21.67 +56:30:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252692_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252692_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:00:49.25 +55:18:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252821_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 252821_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:18.80 +52:49:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253019_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 253019_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:41:28.16 +56:35:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 253054_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:23:18.76 +57:35:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253161_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 253161_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253478_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 253478_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254527_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
Preparing report for the candidate 254527_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255015_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 255015_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:08:51.59 +57:52:54.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255644_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 255644_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:33:18.69 +50:11:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257194_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 257194_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:28:30.77 +55:47:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 3.730 2186637673686539904 307.12706566597 +55.79234061618 14.7331 14.1001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219520_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 219520_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:39:48.58 +52:53:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68406_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 68406_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:35:54.83 +54:49:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76678_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 76678_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:51:26.99 +53:56:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87903_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 87903_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 20:32:45.09 +54:17:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27975_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 27975_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:24:40.27 +57:18:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63125_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 63125_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:39:02.86 +54:58:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180642_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 180642_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:18:22.05 +49:57:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220363_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433
The candidate 220363_fd_Cyg-02-Q2b1x1_2026-03-21_04-56-16_20.00sec_-15.00C_LIGHT_0433 did not pass the final checks
**** FOUND 21:34:23.87 +50:03:15.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 372s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:43:14.19 +50:43:55.0
20:35:30.11 +52:07:55.8
20:57:27.49 +54:18:58.1
20:42:18.85 +52:16:49.3
20:43:08.95 +55:29:08.3
20:54:56.77 +56:35:37.8
20:39:06.57 +54:38:19.6
21:34:53.09 +51:05:34.3
21:49:35.57 +55:09:44.6
20:35:10.94 +53:32:42.7
20:28:40.48 +55:01:23.2
21:38:05.59 +50:31:30.8
21:45:36.07 +52:09:23.4
20:33:37.60 +52:36:19.9
21:37:52.75 +51:04:04.6
20:42:40.24 +51:01:42.1
21:48:19.07 +53:05:55.7
21:15:32.00 +54:44:03.3
20:36:53.67 +52:45:04.1
21:22:04.42 +50:47:53.9
20:44:31.87 +55:20:08.5
20:30:37.90 +50:36:55.4
21:27:53.97 +57:03:25.2
20:53:08.97 +50:43:26.3
########### Completed Cyg-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:43:14.19 +50:43:55.0
20:35:30.11 +52:07:55.8
20:57:27.49 +54:18:58.1
20:42:18.85 +52:16:49.3
20:43:08.95 +55:29:08.3
20:54:56.77 +56:35:37.8
20:39:06.57 +54:38:19.6
21:34:53.09 +51:05:34.3
21:49:35.57 +55:09:44.6
20:35:10.94 +53:32:42.7
20:28:40.48 +55:01:23.2
21:38:05.59 +50:31:30.8
21:45:36.07 +52:09:23.4
20:33:37.60 +52:36:19.9
21:37:52.75 +51:04:04.6
20:42:40.24 +51:01:42.1
21:48:19.07 +53:05:55.7
21:15:32.00 +54:44:03.3
20:36:53.67 +52:45:04.1
21:22:04.42 +50:47:53.9
20:44:31.87 +55:20:08.5
20:30:37.90 +50:36:55.4
21:27:53.97 +57:03:25.2
20:53:08.97 +50:43:26.3
###################################################################################
20:43:14.19 +50:43:55.0 -- not an asteroid (will add it to exclusion list)
20:35:30.11 +52:07:55.8 -- not an asteroid (will add it to exclusion list)
20:57:27.49 +54:18:58.1 -- not an asteroid (will add it to exclusion list)
20:42:18.85 +52:16:49.3 -- not an asteroid (will add it to exclusion list)
20:43:08.95 +55:29:08.3 -- not an asteroid (will add it to exclusion list)
20:54:56.77 +56:35:37.8 -- not an asteroid (will add it to exclusion list)
20:39:06.57 +54:38:19.6 -- not an asteroid (will add it to exclusion list)
21:34:53.09 +51:05:34.3 -- not an asteroid (will add it to exclusion list)
21:49:35.57 +55:09:44.6 -- not an asteroid (will add it to exclusion list)
20:35:10.94 +53:32:42.7 -- not an asteroid (will add it to exclusion list)
20:28:40.48 +55:01:23.2 -- not an asteroid (will add it to exclusion list)
21:38:05.59 +50:31:30.8 -- not an asteroid (will add it to exclusion list)
21:45:36.07 +52:09:23.4 -- not an asteroid (will add it to exclusion list)
20:33:37.60 +52:36:19.9 -- not an asteroid (will add it to exclusion list)
21:37:52.75 +51:04:04.6 -- not an asteroid (will add it to exclusion list)
20:42:40.24 +51:01:42.1 -- not an asteroid (will add it to exclusion list)
21:48:19.07 +53:05:55.7 -- not an asteroid (will add it to exclusion list)
21:15:32.00 +54:44:03.3 -- not an asteroid (will add it to exclusion list)
20:36:53.67 +52:45:04.1 -- not an asteroid (will add it to exclusion list)
21:22:04.42 +50:47:53.9 -- not an asteroid (will add it to exclusion list)
20:44:31.87 +55:20:08.5 -- not an asteroid (will add it to exclusion list)
20:30:37.90 +50:36:55.4 -- not an asteroid (will add it to exclusion list)
21:27:53.97 +57:03:25.2 -- not an asteroid (will add it to exclusion list)
20:53:08.97 +50:43:26.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:28:40.48 +55:01:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:37.90 +50:36:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:37.60 +52:36:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:10.94 +53:32:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:30.11 +52:07:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:53.67 +52:45:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:06.57 +54:38:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:18.85 +52:16:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:40.24 +51:01:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:08.95 +55:29:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:14.19 +50:43:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:31.87 +55:20:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:08.97 +50:43:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.77 +56:35:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:27.49 +54:18:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:32.00 +54:44:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:04.42 +50:47:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:53.97 +57:03:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:53.09 +51:05:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:52.75 +51:04:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:05.59 +50:31:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:36.07 +52:09:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:19.07 +53:05:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:49:35.57 +55:09:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:28:40.48 +55:01:23.2 -- not a known variable star
20:30:37.90 +50:36:55.4 -- not a known variable star
20:33:37.60 +52:36:19.9 -- not a known variable star
20:35:10.94 +53:32:42.7 -- not a known variable star
20:35:30.11 +52:07:55.8 -- not a known variable star
20:36:53.67 +52:45:04.1 -- not a known variable star
20:39:06.57 +54:38:19.6 -- not a known variable star
20:42:18.85 +52:16:49.3 -- not a known variable star
20:42:40.24 +51:01:42.1 -- not a known variable star
20:43:08.95 +55:29:08.3 -- not a known variable star
20:43:14.19 +50:43:55.0 -- not a known variable star
20:44:31.87 +55:20:08.5 -- not a known variable star
20:53:08.97 +50:43:26.3 -- not a known variable star
20:54:56.77 +56:35:37.8 -- a known variable star
20:57:27.49 +54:18:58.1 -- a known variable star
21:15:32.00 +54:44:03.3 -- not a known variable star
21:22:04.42 +50:47:53.9 -- a known variable star
21:27:53.97 +57:03:25.2 -- not a known variable star
21:34:53.09 +51:05:34.3 -- not a known variable star
21:37:52.75 +51:04:04.6 -- a known variable star
21:38:05.59 +50:31:30.8 -- a known variable star
21:45:36.07 +52:09:23.4 -- a known variable star
21:48:19.07 +53:05:55.7 -- not a known variable star
21:49:35.57 +55:09:44.6 -- not a known variable star
Found 18 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
24 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
20:28:40.48 +55:01:23.2
20:30:37.90 +50:36:55.4
20:33:37.60 +52:36:19.9
20:35:10.94 +53:32:42.7
20:35:30.11 +52:07:55.8
20:36:53.67 +52:45:04.1
20:39:06.57 +54:38:19.6
20:42:18.85 +52:16:49.3
20:42:40.24 +51:01:42.1
20:43:08.95 +55:29:08.3
20:43:14.19 +50:43:55.0
20:44:31.87 +55:20:08.5
20:53:08.97 +50:43:26.3
20:54:56.77 +56:35:37.8
20:57:27.49 +54:18:58.1
21:15:32.00 +54:44:03.3
21:22:04.42 +50:47:53.9
21:27:53.97 +57:03:25.2
21:34:53.09 +51:05:34.3
21:37:52.75 +51:04:04.6
21:38:05.59 +50:31:30.8
21:45:36.07 +52:09:23.4
21:48:19.07 +53:05:55.7
21:49:35.57 +55:09:44.6
20:57:13.44 +53:46:56.1
21:18:57.74 +50:33:23.6
21:07:37.15 +53:32:15.9
21:55:54.72 +57:02:48.5
21:31:32.39 +55:04:53.9
21:05:34.43 +54:04:41.3
21:28:44.02 +51:08:11.4
21:13:05.38 +50:25:30.0
21:20:19.36 +54:18:33.9
21:12:20.52 +52:27:00.3
21:12:27.34 +54:16:00.6
21:06:46.17 +54:00:23.6
21:18:18.89 +52:01:38.8
21:40:36.81 +54:16:38.1
21:23:38.95 +50:02:31.5
21:51:55.12 +55:14:19.1
20:34:15.37 +49:44:54.2
20:28:30.77 +55:47:29.5
21:08:51.59 +57:52:54.0
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461120.91363054 -observatory 500
22:37:54.15 -07:44:10.3 Mercury (1.0mag)
01:08:27.51 +06:21:25.0 Venus (-3.9mag)
23:04:22.51 -07:06:44.8 Mars (1.2mag)
07:04:49.25 +22:57:56.6 Jupiter (-2.3mag)
00:17:32.29 -00:24:57.1 Saturn (0.9mag)
03:42:59.90 +19:32:05.1 Uranus (5.8mag)
00:07:20.85 -00:37:39.9 Neptune (7.8mag)
20:32:02.55 -22:53:44.3 Pluto (14.5mag)
01:51:54.08 +15:58:19.0 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Mar 21 05:00 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461120.91363054:
07:04:48.72 +22:57:54.3 Io (5.6mag)
07:04:37.41 +22:58:21.0 Europa (5.7mag)
07:04:27.29 +22:58:37.6 Ganymede (5.2mag)
07:04:12.15 +22:59:01.7 Callisto (6.4mag)
07:08:50.48 +22:59:18.9 Himalia (15.2mag)
07:04:49.33 +22:57:53.5 Thebe (16.0mag)
07:08:25.84 +23:22:46.7 Elara (17.2mag)
07:01:58.87 +23:51:24.4 Pasiphae (17.2mag)
07:13:36.36 +22:52:28.5 Carme (18.3mag)
00:17:27.80 -00:24:55.0 Titan (8.8mag)
00:17:38.06 -00:24:54.8 Rhea (10.1mag)
00:18:01.67 -00:22:53.6 Iapetus (11.5mag)
00:17:47.55 -00:25:01.3 Hyperion (14.8mag)
00:19:26.21 -00:13:43.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 21 05:00 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461120.91363054:
12:53:20.34 +08:24:55.6 JWST
16:59:25.96 +44:33:23.0 Chandra
08:54:53.20 -46:29:39.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 21 05:00 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461120.91363054 -observatory 500
18:35:45.60 -27:28:48.2 14.0mag P/2010 H2 (Vales)
04:51:21.35 -71:00:35.4 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:45.54 +31:17:59.6 17.0mag C/2017 K2 (PANSTARRS)
17:29:42.05 +07:27:16.9 17.6mag C/2021 G2 (ATLAS)
23:01:43.18 +28:26:38.6 16.9mag C/2022 E2 (ATLAS)
04:00:55.39 +25:18:22.6 15.7mag C/2022 N2 (PANSTARRS)
09:01:50.90 +31:27:54.8 16.0mag C/2022 QE78 (ATLAS)
08:30:09.42 -03:07:31.7 17.2mag C/2022 R6 (PANSTARRS)
18:56:30.25 +16:19:37.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:18.95 -11:50:30.7 17.6mag P/2023 B1 (PANSTARRS)
09:24:11.06 -16:15:17.5 17.4mag C/2023 F3 (ATLAS)
21:22:18.83 +61:42:38.4 17.4mag C/2023 H5 (Lemmon)
19:33:05.61 -03:31:18.3 14.5mag C/2023 R1 (PANSTARRS)
21:36:42.43 +82:53:35.1 17.7mag C/2023 X2 (Lemmon)
06:15:15.93 +63:46:50.1 16.8mag C/2024 A1 (ATLAS)
04:07:44.23 +05:30:36.5 9.1mag C/2024 E1 (Wierzchos)
11:22:17.79 +02:48:45.2 18.0mag C/2024 G2 (ATLAS)
16:32:07.92 +02:13:46.6 17.5mag C/2024 G6 (ATLAS)
20:10:16.53 +08:51:31.6 14.9mag C/2024 J3 (ATLAS)
03:05:01.03 -26:34:52.4 16.5mag C/2024 T5 (ATLAS)
04:57:46.99 +52:28:28.2 17.6mag C/2025 J1 (Borisov)
15:12:39.53 +18:01:29.0 14.4mag C/2025 L1 (ATLAS)
02:49:02.52 -22:37:54.1 17.6mag C/2025 Q3 (ATLAS)
22:33:10.61 +19:02:37.8 12.4mag C/2025 R3 (PANSTARRS)
13:04:54.62 +01:20:22.4 17.6mag C/2025 Y1 (ATLAS)
02:08:46.01 -06:06:46.8 14.0mag C/2026 A1 (MAPS)
22:40:18.20 +31:10:05.9 13.7mag C/2026 B2 (Sun-Gao)
17:52:52.58 -10:49:45.9 13.3mag 10P/Tempel
15:26:34.98 +05:06:56.6 11.8mag 24P/Schaumasse
11:11:49.44 -02:27:54.4 15.6mag 29P/Schwassmann-Wachmann
17:44:05.16 -10:37:47.6 17.3mag 40P/Vaisala
10:44:56.13 -06:31:26.0 16.4mag 43P/Wolf-Harrington
01:09:34.82 +12:59:51.5 17.0mag 47P/Ashbrook-Jackson
06:29:08.78 +42:16:02.0 17.1mag 63P/Wild
22:54:46.68 -14:41:17.0 15.7mag 65P/Gunn
02:59:25.23 +11:29:40.1 15.9mag 76P/West-Kohoutek-Ikemura
00:10:22.97 +03:07:51.6 14.6mag 78P/Gehrels
21:40:10.16 -16:38:13.4 14.5mag 88P/Howell
01:01:48.33 +13:20:59.6 15.2mag 93P/Lovas
04:11:13.24 +30:42:46.6 16.5mag 123P/West-Hartley
08:07:54.53 +50:04:53.2 16.2mag 124P/Mrkos
01:54:55.97 +11:24:12.5 16.4mag 128P/Shoemaker-Holt
01:58:10.92 +11:05:31.3 17.4mag 131P/Mueller
23:21:54.41 +03:15:49.8 12.9mag 141P/Machholz
23:32:01.94 -04:18:00.4 13.0mag 141P-A/Machholz
22:32:31.18 -06:52:23.5 16.0mag 141P-D/Machholz
23:51:32.83 -13:57:30.6 15.5mag 162P/SidingSpring
10:39:04.01 +32:01:59.3 17.5mag 164P/Christensen
05:50:26.35 +24:44:09.5 17.5mag 198P/ODAS
15:32:49.16 -03:19:01.9 16.9mag 210P/Christensen
20:13:24.15 -17:27:35.1 17.2mag 218P/LINEAR
16:59:42.47 -16:38:26.4 16.3mag 235P/LINEAR
04:42:13.67 +32:03:15.2 16.3mag 240P/NEAT
07:29:56.80 -08:19:02.5 17.5mag 242P/Spahr
15:48:33.24 +05:08:05.3 17.7mag 391P/Kowalski
07:28:01.71 +21:06:51.7 17.5mag 450P/LONEOS
05:01:27.41 +46:35:25.8 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 21 05:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 21 05:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 21 05:00 tocp_transients_list.txt