This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 11.19 18:07:29.04 +64:52:17.2
94.46563 29.00375 galactic Dra Second-epoch detections are separated by 4.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161500123448459264 | 18:07:30.56 +64:52:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161500123448459264,2461098.7226,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161500123448459264 20260227.2226 11.19CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:29.04 +64:52:17.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 10.47 18:06:47.09 +64:57:01.9
94.55227 29.08128 galactic Dra Second-epoch detections are separated by 3.7" and 6.9 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 | Gaia DR3 2161502734788130688 | 18:06:48.44 +64:57:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161502734788130688,2461098.7226,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161502734788130688 20260227.2226 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:47.09 +64:57:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 10.87 18:07:58.48 +65:05:12.1
94.71415 28.96176 galactic Dra Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161498542900078848 | 18:07:59.46 +65:05:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161498542900078848,2461098.7226,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161498542900078848 20260227.2226 10.87CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:58.48 +65:05:12.1 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 11.76 18:08:00.38 +64:54:53.7
94.51822 28.95043 galactic Dra Second-epoch detections are separated by 3.9" and 6.9 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 | Gaia DR3 2161490159123804160 | 18:08:01.88 +64:54:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161490159123804160,2461098.7226,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161490159123804160 20260227.2226 11.76CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:00.38 +64:54:53.7 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 12.38 18:08:00.38 +65:00:23.2
94.62271 28.95473 galactic Dra Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161496751897920384 | 18:08:01.36 +65:00:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161496751897920384,2461098.7226,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161496751897920384 20260227.2226 12.38CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:00.38 +65:00:23.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 12.46 18:07:12.60 +64:59:30.2
94.60156 29.03812 galactic Dra Second-epoch detections are separated by 3.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161503147105088896 | 18:07:13.76 +64:59:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161503147105088896,2461098.7226,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161503147105088896 20260227.2226 12.46CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:12.60 +64:59:30.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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,2461098.7226,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.2226 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:32.40 +64:52:55.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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 2161480023001051136,2461098.7226,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2161480023001051136 20260227.2226 13.21CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:30.00 +64:50:14.3 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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,2461098.7226,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.2226 13.37CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:07.36 +64:50:20.4 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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,2461098.7226,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.2226 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:55.90 +64:49:39.3 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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,2461098.7226,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.2226 13.93CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:27.23 +64:51:53.6 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_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: 2461033.00878898 23.12.2025 12:12:29.368 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
First image: 2461033.00878898 23.12.2025 12:12:29.368 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Last image: 2461098.72291727 27.02.2026 05:20:50.052 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 3 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): 9705
Objects passed selection criteria: 9682
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: 7787
Average stars matched: 7643 (98.1508 %)
Memory usage VmPeak: 115648 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 23:23:05 CST 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: 2461033.00878898 23.12.2025 12:12:29.368 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
First image: 2461033.00878898 23.12.2025 12:12:29.368 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Last image: 2461098.72291727 27.02.2026 05:20:50.052 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 12 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): 55696
Objects passed selection criteria: 55591
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 47870
Average stars matched: 46725.8 (97.6097 %)
Memory usage VmPeak: 156592 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 23:24:12 CST 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
SExtractor catalog cache: saved Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat to cache
SExtractor catalog cache: saved Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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: 2461098.72227229
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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits exists and is non-empty
Saving wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits to local_wcs_cache/
'wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits' -> 'local_wcs_cache/wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits'
wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits exists and is non-empty
Saving wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits to local_wcs_cache/
'wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits' -> 'local_wcs_cache/wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits'
wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits exists and is non-empty
Saving wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits to local_wcs_cache/
'wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits'
wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits exists and is non-empty
Saving wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits to local_wcs_cache/
'wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits' -> 'local_wcs_cache/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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 16:47:49.322 +69:59:37.51
Second-epoch image center 16:48:11.610 +69:59:23.20
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:47:49.322 +69:59:37.51
Second-epoch image center 16:48:08.091 +70:00:02.03
Angular distance between the image centers 0.03 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 16:48:11.610 +69:59:23.20
Second-epoch second image center 16:48:08.091 +70:00:02.03
Angular distance between the image centers 0.01189 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits &> /tmp/tmp.My6Wl596PX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits &> /tmp/tmp.J9YH6cz5AP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.zOFUTqV9UC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits &> /tmp/tmp.O8O3dFdNRI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
Found non-empty wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
The reference image (wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits) and catalog (wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat) found
'wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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 6443 out of 10241 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.854814
a=0.000000 b=1.000000 c=22.854814
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
2.1 pix Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
2.1 pix fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
2.1 pix fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Limiting magnitude estimates:
15.2 mag. Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
15.2 mag. Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
14.4 mag. fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
14.4 mag. fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.4 (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.My6Wl596PX (6) ############
Parsing command line arguments...
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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits' -> 'wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS_IMAGE_NAME=wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS-calibrated image found: wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Checking if the catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits alredy exist and is non-empty...
Catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS catalog name: wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=717, passed=10241
Got 10241 stars (including 9513 good ones) from the SExtractor catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
util/solve_plate_with_UCAC5 got 10241 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits -region wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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.J9YH6cz5AP (6) ############
Parsing command line arguments...
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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits' -> 'wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS_IMAGE_NAME=wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS-calibrated image found: wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
Checking if the catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits alredy exist and is non-empty...
Catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS catalog name: wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=726, passed=10266
Got 10266 stars (including 9534 good ones) from the SExtractor catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat
util/solve_plate_with_UCAC5 got 10266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits -region wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.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.zOFUTqV9UC (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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=445, passed=5420
Got 5420 stars (including 4967 good ones) from the SExtractor catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 5420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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: 0.35"
Estimated accuracy of the plate solution: 0.34"
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_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.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.O8O3dFdNRI (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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Checking if the catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS catalog name: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=5390
Got 5390 stars (including 4930 good ones) from the SExtractor catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat
util/solve_plate_with_UCAC5 got 5390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
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_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits -region wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits'
Saving fully-calibrated image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits'
Preparing the HTML report for the field Dra-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20559.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20559_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 20559_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07822_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 07822_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:19:25.22 +72:40:48.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Dra-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:07:29.04 +64:52:17.2
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
SExtractor catalog cache: saved Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat to cache
SExtractor catalog cache: saved Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Creating symlink local_wcs_cache/wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits exists and is non-empty
wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits exists and is non-empty
wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits exists and is non-empty
wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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 16:47:49.322 +69:59:37.51
Second-epoch image center 16:48:11.610 +69:59:23.20
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:47:49.322 +69:59:37.51
Second-epoch image center 16:48:08.091 +70:00:02.03
Angular distance between the image centers 0.03 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 16:48:11.610 +69:59:23.20
Second-epoch second image center 16:48:08.091 +70:00:02.03
Angular distance between the image centers 0.01189 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits &> /tmp/tmp.yQ2wTLO9Rn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits &> /tmp/tmp.1AbS7xpm8q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.zgyF2dphsa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits &> /tmp/tmp.lleWjkpYCT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
Found non-empty wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits and wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
The reference image (wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits) and catalog (wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat) found
'wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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 6627 out of 60234 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.730261
a=0.000000 b=1.000000 c=22.730261
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
2.0 pix Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
2.0 pix fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
1.9 pix fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Limiting magnitude estimates:
15.4 mag. Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
15.4 mag. Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
14.5 mag. fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
14.5 mag. fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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.yQ2wTLO9Rn (6) ############
Parsing command line arguments...
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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits' -> 'wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS_IMAGE_NAME=wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS-calibrated image found: wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
Checking if the catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits alredy exist and is non-empty...
Catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits
WCS catalog name: wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3188, passed=60223
Got 60223 stars (including 56935 good ones) from the SExtractor catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat
util/solve_plate_with_UCAC5 got 60223 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 961 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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits -region wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.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.1AbS7xpm8q (6) ############
Parsing command line arguments...
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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits' -> 'wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS_IMAGE_NAME=wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS-calibrated image found: wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
Checking if the catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits alredy exist and is non-empty...
Catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat corresponding to the image wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits
WCS catalog name: wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=3106, passed=59789
Got 59789 stars (including 56585 good ones) from the SExtractor catalog wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat
util/solve_plate_with_UCAC5 got 59789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
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_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits -region wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-04-Q1b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.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.zgyF2dphsa (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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1369, passed=36230
Got 36230 stars (including 34799 good ones) from the SExtractor catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 36230 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
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_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.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.lleWjkpYCT (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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Checking if the catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
WCS catalog name: wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1342, passed=36351
Got 36351 stars (including 34942 good ones) from the SExtractor catalog wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat
util/solve_plate_with_UCAC5 got 36351 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
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_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits -region wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits
Saving fully-calibrated image wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.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_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits
Preparing the HTML report for the field Dra-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out74314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out74346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74589.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74314_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74314_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:04:49.69 +71:33:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.124 1651773542197413504 256.20606706846 +71.56041970019 14.3820 13.8362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74324_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74324_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 15:01:42.85 +71:21:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74326_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74326_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:52:05.57 +65:26:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.945 1441042036971398016 268.02380395116 +65.44914312328 13.2021 12.6993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74328_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74328_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:24:39.31 +68:29:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 0.814 1649475597254671232 246.16408599034 +68.49636548253 11.1575 10.5040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74346_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74346_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74352_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74352_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74356_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74356_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:07:29.09 +64:52:17.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74372_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74372_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:27:55.23 +68:48:05.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74373_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74373_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74380_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74380_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:06:37.47 +67:48:56.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74383_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74383_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:07:53.96 +64:58:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74385_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74385_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 15:52:10.27 +64:52:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.866 1641186069856315008 238.04335479730 +64.87652961926 12.2424 11.5670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74388_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74388_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74394_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74394_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:06:51.89 +66:09:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74396_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74396_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74397_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74397_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:06:53.72 +73:31:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.161 2266977064174710784 271.72287937362 +73.53028689244 12.7671 12.2813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74401_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74401_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:27:32.56 +73:16:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.026 2267063788154662144 276.88606819458 +73.26951040498 12.5943 12.1089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74410_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74410_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:15:26.56 +68:46:15.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74411_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74411_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74412_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74412_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:08:26.02 +65:44:20.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74416_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74416_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:19:25.82 +71:31:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74425_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74425_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:12:23.30 +70:52:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74440_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74440_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:30:48.37 +70:32:20.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74464_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74464_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74466_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74466_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:32:57.71 +74:38:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74467_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74467_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:01:19.91 +73:20:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.835 1655175568613040128 255.33356510428 +73.33512573602 13.3316 12.8583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74476_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74476_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:07:26.01 +65:03:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74479_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74479_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74485_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74485_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:34:53.97 +66:55:28.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74495_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74495_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:04:04.28 +65:06:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 5.549 2161554029581188608 271.02128448288 +65.10801533198 13.2917 12.8691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74497_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74497_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:55:51.41 +70:09:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74510_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74510_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:49:46.57 +70:56:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74517_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74517_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 15:30:17.22 +70:22:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74518_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74518_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:52:48.24 +64:54:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.672 1635002760059096832 253.20085887853 +64.90437135626 13.8982 13.2023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74525_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74525_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:55:59.38 +70:09:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74526_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74526_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:45:27.91 +70:16:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74528_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74528_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:39:27.96 +70:36:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74532_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74532_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:38:07.44 +65:25:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.850 1635949473930301056 249.53043856204 +65.42731281389 13.7142 13.1826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74534_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74534_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:39:40.59 +66:20:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.629 1636258677216101376 249.91869908321 +66.33710253242 13.8308 13.2385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74535_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74535_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:21:53.89 +71:43:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.262 1653338490841586432 245.47544975944 +71.73014355682 13.8997 13.4271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74544_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74544_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74551_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74551_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:00:46.28 +68:03:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.321 1646629614485564416 240.19529772681 +68.05128458137 14.0118 13.5767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74557_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74557_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:33:23.38 +67:17:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.441 1634163386010283008 263.34843075717 +67.29930453271 13.6645 13.1724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74565_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74565_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:23:22.61 +73:37:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74570_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74570_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:50:24.02 +73:27:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74575_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74575_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:05:09.73 +70:15:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.578 1647137932455271296 241.29258981310 +70.26551953102 14.1336 13.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74578_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74578_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:38:00.10 +67:24:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74581_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74581_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:30:24.20 +67:20:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.845 1648416252162130048 247.60179066619 +67.33767194912 13.9845 13.4773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74589_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
Preparing report for the candidate 74589_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74590_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74590_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 16:53:45.29 +65:38:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74594_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74594_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:10:36.12 +72:40:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.685 1652095389866954112 257.65230687712 +72.67290534989 13.9231 13.4211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74638_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 74638_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 17:07:15.99 +69:23:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.964 1649068468715270528 256.81677184236 +69.39218197077 14.4094 13.8425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52114_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 52114_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks
**** FOUND 18:19:25.18 +72:40:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70397_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215
The candidate 70397_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215 did not pass the final checks