This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2816* 16 21 55.80 -01 03 31.0 12.9 U Ser 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
VARIABLE_NAME,2461129.7816,12.91,0.05,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
VARIABLE_NAME 20260330.2816 12.91CV 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:21:55.80 -01:03:31.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2816* 16 08 17.74 -02 46 12.7 13.2 U Ser 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
VARIABLE_NAME,2461129.7816,13.25,0.05,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
VARIABLE_NAME 20260330.2816 13.25CV 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:08:17.74 -02:46:12.7 ;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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2816* 16 16 02.41 +00 41 54.1 13.8 U Ser 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
VARIABLE_NAME,2461129.7816,13.84,0.05,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
VARIABLE_NAME 20260330.2816 13.84CV 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:16:02.41 -00:41:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.2816 2461129.7816 12.64 16:41:18.17 +00:58:19.7
17.66445 29.09768 galactic Oph Second-epoch detections are separated by 1.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:41:18.17 +00:58:19.7 (user input) | T | P | (position from user input) J-Ks=0.273+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.7816,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.2816 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:18.17 +00:58:19.7 ;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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.2816 2461129.7816 12.90 16:14:03.00 +00:19:53.0
12.76935 34.53391 galactic Ser Second-epoch detections are separated by 0.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:14:03.00 +00:19:53.0 (user input) | T | P | (position from user input) J-Ks=0.835+/-0.030 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2816* 16 14 03.00 +00 19 53.0 12.9 U Ser 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,2461129.7816,12.90,0.05,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 20260330.2816 12.90CV 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:03.00 +00:19:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20_00sec_-10_00C_LIGHT_0273_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20_00sec_-14_90C_LIGHT_0504_fits__*pix.png resample_wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20_00sec_-10_00C_LIGHT_0272_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: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
First image: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Last image: 2461129.78189043 30.03.2026 06:45:45.333 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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): 6979
Objects passed selection criteria: 6951
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4891
Average stars matched: 4747.75 (97.0712 %)
Memory usage VmPeak: 113564 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 Mon Mar 30 01:49:35 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: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
First image: 2461094.01320807 22.02.2026 12:18:51.177 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Last image: 2461129.78189043 30.03.2026 06:45:45.333 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 256
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 10 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): 46876
Objects passed selection criteria: 46772
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 35721
Average stars matched: 34251.5 (95.8862 %)
Memory usage VmPeak: 150696 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 Mon Mar 30 01:50:23 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat to cache
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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: 2461129.78126487
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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits exists and is non-empty
Saving wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits to local_wcs_cache/
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits exists and is non-empty
Saving wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits to local_wcs_cache/
'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits exists and is non-empty
Saving wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits to local_wcs_cache/
'wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits' -> 'local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits'
wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits exists and is non-empty
Saving wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits to local_wcs_cache/
'wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits' -> 'local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:29.621 -02:01:30.78
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:31.822 -02:00:55.68
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:17:29.621 -02:01:30.78
Second-epoch second image center 16:17:31.822 -02:00:55.68
Angular distance between the image centers 0.01338 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits &> /tmp/tmp.gn7tc04hFR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits &> /tmp/tmp.mzlNu33dKD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits &> /tmp/tmp.oPFGNPzyuz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits &> /tmp/tmp.tgU71dWJrL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
The reference image (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits) and catalog (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat) found
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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 4442 out of 8868 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.923574
a=0.000000 b=1.000000 c=22.923574
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
2.4 pix Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
2.4 pix fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
2.4 pix fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Limiting magnitude estimates:
15.0 mag. Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
15.0 mag. Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
13.7 mag. fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
13.8 mag. fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.9 (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.gn7tc04hFR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, passed=8867
Got 8867 stars (including 8350 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
util/solve_plate_with_UCAC5 got 8867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 970 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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.mzlNu33dKD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=557, passed=8941
Got 8941 stars (including 8375 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
util/solve_plate_with_UCAC5 got 8941 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.45"
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_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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.oPFGNPzyuz (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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=224, passed=2958
Got 2958 stars (including 2729 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat
util/solve_plate_with_UCAC5 got 2958 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.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.tgU71dWJrL (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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=248, passed=2974
Got 2974 stars (including 2723 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat
util/solve_plate_with_UCAC5 got 2974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
Saving fully-calibrated image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits'
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits'
Preparing the HTML report for the field Ser-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20489_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 20489_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:07:08.15 -00:18:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20546_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 20546_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:54.64 -03:55:37.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ser-06-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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat to cache
SExtractor catalog cache: saved Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Creating symlink local_wcs_cache/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits exists and is non-empty
wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits exists and is non-empty
wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits exists and is non-empty
wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:29.621 -02:01:30.78
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:09.440 -02:00:32.87
Second-epoch image center 16:17:31.822 -02:00:55.68
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:17:29.621 -02:01:30.78
Second-epoch second image center 16:17:31.822 -02:00:55.68
Angular distance between the image centers 0.01338 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/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits &> /tmp/tmp.sk52SCFJaM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits &> /tmp/tmp.XtqV2aeXpj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits &> /tmp/tmp.s2JiAttyGu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits &> /tmp/tmp.z2FNJjoB6g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
Found non-empty wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits and wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
The reference image (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits) and catalog (wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat) found
'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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 4513 out of 57255 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756312
a=0.000000 b=1.000000 c=22.756312
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
2.2 pix Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
2.1 pix fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
2.1 pix fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Limiting magnitude estimates:
15.2 mag. Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
15.2 mag. Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
13.9 mag. fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
14.0 mag. fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.4 (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.sk52SCFJaM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=3363, passed=57246
Got 57246 stars (including 53818 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat
util/solve_plate_with_UCAC5 got 57246 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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: 0.45"
Estimated accuracy of the plate solution: 0.44"
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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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.XtqV2aeXpj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits' -> 'wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS_IMAGE_NAME=wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS-calibrated image found: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Checking if the catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits alredy exist and is non-empty...
Catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat corresponding to the image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
WCS catalog name: wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3390, passed=57768
Got 57768 stars (including 54311 good ones) from the SExtractor catalog wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat
util/solve_plate_with_UCAC5 got 57768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
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_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits -region wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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.s2JiAttyGu (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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=726, passed=23791
Got 23791 stars (including 23032 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat
util/solve_plate_with_UCAC5 got 23791 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.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.z2FNJjoB6g (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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS_IMAGE_NAME=wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS-calibrated image found: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Checking if the catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat corresponding to the image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
WCS catalog name: wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=757, passed=23806
Got 23806 stars (including 23005 good ones) from the SExtractor catalog wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat
util/solve_plate_with_UCAC5 got 23806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits -region wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_Ser-06-Q2b1x1_2026-02-22_06-18-51_20.00sec_-14.90C_LIGHT_0504.fits
Saving fully-calibrated image wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_Ser-06-Q2b1x1_2026-02-22_06-19-39_20.00sec_-15.00C_LIGHT_0505.fits
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-44-51_20.00sec_-10.00C_LIGHT_0272.fits
Saving fully-calibrated image wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.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_2026-03-30_CI_Ser-06-Q2b1x1_014724_TTUQ2b1x1_24199_q7iurDnO/wcs_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273.fits
Preparing the HTML report for the field Ser-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out71845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out39710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72867.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 71845_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71845_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:37:32.40 +00:42:34.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 71846_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71846_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:39.11 +00:22:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71847_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71847_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:04.16 +01:25:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71848_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71848_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:16:22.36 -01:37:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.243 4407056841394389120 244.09377100970 -01.62976342405 13.4469 12.8308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71850_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71850_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:00:28.02 -01:01:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.216 4409232942407746944 240.11669206096 -01.02965475016 12.6739 12.0095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71852_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71852_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:38:47.62 -02:30:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71857_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71857_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:46.15 -01:42:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.742 4382063322888821120 250.44209866478 -01.70787181883 12.2094 11.4893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71858_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71858_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 15:50:39.81 -05:45:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71994_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 71994_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:43.00 -03:59:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.728 4354541584771982208 250.17936202559 -03.99064057663 10.7337 9.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72003_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72003_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:54.64 -03:55:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72022_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72022_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:31.83 +02:06:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 0.621 4384233969297702912 250.38248745443 +02.10486795018 11.3657 10.9230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72027_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72027_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:30:56.20 +01:57:03.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 72033_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72033_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:26.19 +02:09:05.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)
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Considering the candidate 72048_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72048_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:56.54 -03:42:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72078_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72078_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:43.50 +01:45:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72091_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72091_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:21.26 -03:40:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72092_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72092_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:45.77 +01:47:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.144 4384171537653181568 250.44074717459 +01.78837902079 11.5526 10.8926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72132_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72132_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:15.67 -02:30:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72152_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72152_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:16.77 -03:07:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72164_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72164_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:28:28.69 +00:38:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72213_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72213_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:28.54 +01:56:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.977 4384222561864721920 250.36873038113 +01.93780239340 12.0551 11.5645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72259_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72259_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:33.87 -03:57:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72272_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72272_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:52.76 +01:01:04.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 72276_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72276_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:13.24 -02:58:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72297_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72297_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:02:58.22 -05:49:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72312_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72312_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:55.89 -03:33:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72351_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72351_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:19.81 -03:58:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72361_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72361_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:03.45 -03:30:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72384_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72384_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:02:06.21 -00:48:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72398_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72398_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:17.69 -02:49:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72400_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72400_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:52.93 +01:26:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.811 4384124219996935808 250.47065285126 +01.44596285702 12.8869 12.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72407_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72407_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:12.13 -03:46:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72413_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72413_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:53.37 +01:52:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.689 4384174148993168128 250.47218345039 +01.86977682567 12.8489 12.3401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72415_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72415_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 15:55:30.75 -05:50:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72422_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
Preparing report for the candidate 72422_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
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Considering the candidate 72426_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72426_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:24.64 -02:37:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72461_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72461_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:10.29 -03:03:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72466_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72466_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:24.05 -02:25:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72470_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72470_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:15.38 -03:49:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72479_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72479_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:03.62 +02:11:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.200 4384247060358041856 250.26509765040 +02.19138703645 12.7369 12.2113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72493_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72493_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:26:54.64 -03:00:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72503_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72503_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:32.49 -03:41:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72541_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72541_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:06.67 +01:51:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.514 4384220362841158656 250.27820412454 +01.86111069175 13.0278 12.3599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72543_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72543_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:13.75 -02:50:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72551_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72551_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:50.91 +01:14:58.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 72577_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72577_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:23:23.90 -04:54:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.824 4355864335917347840 245.84947579567 -04.91206330969 13.1340 12.4221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72591_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72591_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:15.03 -03:03:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72593_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72593_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:50.24 +02:05:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72608_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72608_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:52.46 +02:07:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.908 4384234759571681024 250.46834163752 +02.12795475315 13.1705 12.6835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72618_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72618_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:46.06 -03:45:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72631_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72631_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:12.84 -03:55:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72654_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72654_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:17:42.71 -06:07:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72658_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
Preparing report for the candidate 72658_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
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Considering the candidate 72662_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72662_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:00.59 -03:19:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72667_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72667_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:34.16 +01:54:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.601 4384201327546117504 250.14230761972 +01.91135936157 13.2290 12.7231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72742_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72742_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:20:56.94 -00:24:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72828_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 72828_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:27.23 -01:43:36.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 72867_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
Preparing report for the candidate 72867_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
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Considering the candidate 39710_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
Preparing report for the candidate 39710_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
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Considering the candidate 22396_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 22396_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:10.08 -03:07:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67536_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 67536_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 15:54:16.76 -05:45:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22319_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 22319_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:41:12.16 -03:09:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31057_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 31057_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:34:46.89 -01:30:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67383_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 67383_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:40:28.89 +01:20:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30764_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 30764_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:19:37.33 -01:15:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37930_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 37930_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks
**** FOUND 16:07:08.16 -00:18:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53651_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
Preparing report for the candidate 53651_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
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Considering the candidate 41521_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273
The candidate 41521_fd_Ser-06-Q2b1x1_2026-03-30_01-45-45_20.00sec_-10.00C_LIGHT_0273 did not pass the final checks