This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 26.1648 2461125.6648 13.11 07:51:20.00 +50:14:09.2
168.35919 29.84084 galactic Lyn Second-epoch detections are separated by 0.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J117.8374+50.2361 | 07:51:20.00 +50:14:09.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J117.8374+50.2361,2461125.6648,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J117.8374+50.2361 20260326.1648 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:20.00 +50:14:09.2 ;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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.1648 2461125.6648 13.48 08:35:11.52 +51:51:39.4
166.84638 36.80191 galactic UMa Second-epoch detections are separated by 1.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:35:11.52 +51:51:39.4 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1648* 08 35 11.52 +51 51 39.4 13.5 U UMa 9 0
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,2461125.6648,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.1648 13.48CV 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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:11.52 +51:51:39.4 ;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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.1648 2461125.6648 13.80 08:11:11.51 +50:06:09.2
168.89378 32.99014 galactic Lyn Second-epoch detections are separated by 2.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 935130245672734080 | 08:11:14.46 +50:06:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.366+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 935130245672734080,2461125.6648,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 935130245672734080 20260326.1648 13.80CV 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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:11.51 +50:06:09.2 ;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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.1648 2461125.6648 14.20 08:45:00.37 +53:05:33.7
165.18997 38.22448 galactic UMa Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J131.2581+53.0975 | 08:45:00.37 +53:05:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.460+/-0.050 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1648* 08 45 00.37 +53 05 33.7 14.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J131.2581+53.0975,2461125.6648,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J131.2581+53.0975 20260326.1648 14.20CV 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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:45:00.37 +53:05:33.7 ;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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20_00sec_-10_00C_LIGHT_0369_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20_00sec_-9_90C_LIGHT_0368_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: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461125.66505138 26.03.2026 03:57:30.439 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 8332
Objects passed selection criteria: 8312
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 7366.25
Average stars matched: 7212.25 (97.9094 %)
Memory usage VmPeak: 114844 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 23:11:16 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461125.66505138 26.03.2026 03:57:30.439 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 14 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): 48381
Objects passed selection criteria: 48272
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 43197.5
Average stars matched: 41954 (97.1214 %)
Memory usage VmPeak: 151928 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 23:12:02 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.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: 2461125.66448723
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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits'
wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits'
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:16.383 +54:00:00.17
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:17.495 +54:00:27.46
Angular distance between the image centers 0.05 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 08:28:16.383 +54:00:00.17
Second-epoch second image center 08:28:17.495 +54:00:27.46
Angular distance between the image centers 0.00805 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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.K4viVrHKWR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.07XaqME3Md
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits &> /tmp/tmp.tvVYLOfoI2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits &> /tmp/tmp.55EfSzV8ce
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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 20 out of 10732 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854505
a=0.000000 b=1.000000 c=22.854505
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.5 pix fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
2.5 pix fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.4 mag. Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.9 mag. fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
14.9 mag. fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.K4viVrHKWR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=751, passed=10732
Got 10732 stars (including 9968 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 178 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: 10.17"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.34"
Estimated accuracy of the plate solution: 6.08"
Excluding outliers - 202 stars left (next iteration limit 155)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.07XaqME3Md (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=785, passed=10668
Got 10668 stars (including 9872 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 10668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 172 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: 11.19"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.80"
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 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.56"
Estimated accuracy of the plate solution: 7.06"
Excluding outliers - 198 stars left (next iteration limit 150)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.tvVYLOfoI2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=442, passed=7615
Got 7615 stars (including 7167 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat
util/solve_plate_with_UCAC5 got 7615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.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.55EfSzV8ce (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=473, passed=7583
Got 7583 stars (including 7104 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat
util/solve_plate_with_UCAC5 got 7583 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits'
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20570.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20441_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 20441_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:40:49.50 +50:08:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20570_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 20570_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:55:52.70 +55:49:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.294 1036144371781937920 133.96971758761 +55.82446901525 12.4369 12.0124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits exists and is non-empty
wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits exists and is non-empty
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:16.383 +54:00:00.17
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:17.495 +54:00:27.46
Angular distance between the image centers 0.05 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 08:28:16.383 +54:00:00.17
Second-epoch second image center 08:28:17.495 +54:00:27.46
Angular distance between the image centers 0.00805 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/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.SUxH3hwbkN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.m8JRSdjCCi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits &> /tmp/tmp.cdcb2QmHNf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits &> /tmp/tmp.bvppL6VKTp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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 25 out of 60990 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.045955
a=0.000000 b=1.000000 c=22.045955
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.4 pix fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
2.3 pix fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Limiting magnitude estimates:
14.9 mag. Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.9 mag. Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.3 mag. fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
14.3 mag. fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SUxH3hwbkN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3457, passed=60976
Got 60976 stars (including 57414 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 60976 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 172 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: 9.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.46"
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 218 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.39"
Estimated accuracy of the plate solution: 6.55"
Excluding outliers - 189 stars left (next iteration limit 148)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.m8JRSdjCCi (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3501, passed=61060
Got 61060 stars (including 57445 good ones) from the SExtractor catalog wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 61060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 172 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: 10.18"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.40"
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 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.37"
Estimated accuracy of the plate solution: 7.11"
Excluding outliers - 188 stars left (next iteration limit 146)
The image catalog is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.cdcb2QmHNf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2032, passed=40972
Got 40972 stars (including 38895 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat
util/solve_plate_with_UCAC5 got 40972 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.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.bvppL6VKTp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Checking if the catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat corresponding to the image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
WCS catalog name: wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2047, passed=41211
Got 41211 stars (including 39125 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat
util/solve_plate_with_UCAC5 got 41211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits -region wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.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_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_Lyn-02-Q2b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_Lyn-02-Q2b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-56-41_20.00sec_-9.90C_LIGHT_0368.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-02-Q2b1x1_230909_TTUQ2b1x1_30165_Mpt5J9bp/wcs_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369.fits
Preparing the HTML report for the field Lyn-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out74672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out74682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75686.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: 3s
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Considering the candidate 74672_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 74672_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:10:11.13 +52:13:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.729 935592796470968448 122.54564421233 +52.22114628676 14.7974 14.3282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74678_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 74678_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:10:24.83 +52:43:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.533 1031695301058764160 122.60332314328 +52.72698445621 14.4498 13.9443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74682_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
Preparing report for the candidate 74682_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
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Considering the candidate 74918_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 74918_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:08:37.67 +51:32:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74922_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 74922_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:15:57.67 +50:46:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.819 935213808556776448 123.99007320747 +50.77862483295 12.9306 12.5146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 74938_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 74938_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:09:34.24 +55:10:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75005_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75005_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:01:19.04 +54:26:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75037_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75037_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:34:56.85 +50:29:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75109_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75109_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 07:59:07.66 +51:26:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.788 935862486057420544 119.78171450845 +51.44492883909 13.4978 12.9107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75127_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75127_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:04:45.69 +53:40:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.551 1032733343114806016 121.19063346862 +53.67394477091 13.6575 13.1256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75184_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75184_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:39:01.95 +52:57:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75227_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75227_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:20:27.33 +51:18:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.353 1028313649968384512 125.11377624712 +51.30181278862 13.8898 13.3301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75243_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75243_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:25:37.20 +52:15:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.021 1028436417313645824 126.40438161701 +52.25172317930 14.0187 13.4885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75264_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75264_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:31:38.25 +49:54:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.385 1027167443456435200 127.90923707083 +49.90740214713 14.0804 13.6393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75266_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75266_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:25:11.73 +54:30:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75267_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75267_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 09:08:46.33 +51:34:38.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75287_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75287_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:39:51.63 +56:11:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75401_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
Preparing report for the candidate 75401_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
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Considering the candidate 75469_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75469_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:25:31.58 +51:07:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 5.161 1028085570024916352 126.37932360631 +51.12209756583 14.4613 13.7291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75529_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75529_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 07:54:19.35 +52:58:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75580_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75580_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:30:19.30 +54:28:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.671 1033578627038303488 127.58011886825 +54.47948624394 14.5689 14.0255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75588_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
Preparing report for the candidate 75588_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
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Considering the candidate 75625_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 75625_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks
**** FOUND 08:25:52.13 +57:58:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.385 1035297266791858688 126.46577696636 +57.98330536714 14.3071 13.4721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75686_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
Preparing report for the candidate 75686_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
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Considering the candidate 48804_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369
The candidate 48804_fd_Lyn-02-Q2b1x1_2026-03-25_22-57-30_20.00sec_-10.00C_LIGHT_0369 did not pass the final checks