This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:40.20 +10:24:15.7 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:01.69 +10:45:33.0 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.66 08:55:32.59 +10:05:23.9
218.04380 32.10815 galactic Cnc Second-epoch detections are separated by 2.2" and 5.1 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 | 08:55:32.59 +10:05:23.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:32.59 +10:05:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.41 08:55:11.77 +10:18:50.6
217.76169 32.12850 galactic Cnc Second-epoch detections are separated by 4.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 597773307740039936 | 08:55:12.42 +10:18:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 597773307740039936,2461118.8268,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 597773307740039936 20260319.3268 13.41CV 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:11.77 +10:18:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.23 08:55:49.24 +02:02:39.2
226.31506 28.39998 galactic Hya Second-epoch detections are separated by 5.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:55:49.24 +02:02:39.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.23,0.05,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 20260319.3268 13.23CV 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:49.24 +02:02:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_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 19.3268* 09 38 17.37 +07 22 41.8 12.5 U Leo 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,2461118.8268,12.54,0.05,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 20260319.3268 12.54CV 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:38:17.37 +07:22:41.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_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 19.3268* 09 53 40.99 +01 34 45.6 13.6 U Sex 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,2461118.8268,13.55,0.05,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 20260319.3268 13.55CV 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:40.99 +01:34:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8268,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3268 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:14:22.82 +08:10:57.0 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_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 19.3268* 09 36 08.89 +06 52 24.1 14.4 U Leo 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,2461118.8268,14.41,0.05,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 20260319.3268 14.41CV 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:36:08.89 +06:52:24.1 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SW Cnc,2461118.8268,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SW Cnc 20260319.3268 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:59.24 +09:35:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_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: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461118.82704355 19.03.2026 07:50:46.563 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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): 8510
Objects passed selection criteria: 8505
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7968.5
Average stars matched: 7541.25 (94.6383 %)
Memory usage VmPeak: 114060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:02:27 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: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461118.82704355 19.03.2026 07:50:46.563 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 48317
Objects passed selection criteria: 48215
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 45679.8
Average stars matched: 43965.5 (96.2472 %)
Memory usage VmPeak: 147044 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:03:19 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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: 2461118.82648216
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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:54.655 +05:59:02.76
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:52.549 +05:59:06.77
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:54.655 +05:59:02.76
Second-epoch second image center 09:25:52.549 +05:59:06.77
Angular distance between the image centers 0.00880 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.AfN9kDon1l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.dlmay2wZLD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.gsb6OPU0VX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.XerX0Q4frJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 4890 out of 7575 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.831362
a=0.000000 b=1.000000 c=22.831362
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
2.0 pix Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Limiting magnitude estimates:
15.1 mag. Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.1 mag. Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AfN9kDon1l (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=564, passed=7575
Got 7575 stars (including 6996 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 7575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.dlmay2wZLD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=7669
Got 7669 stars (including 7088 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 7669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.gsb6OPU0VX (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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=457, passed=8414
Got 8414 stars (including 7950 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 8414 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.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.XerX0Q4frJ (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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=8454
Got 8454 stars (including 8019 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 8454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20611.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20571_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20571_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:08:59.23 +09:35:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.330 591296123395161728 137.24714575665 +09.59473996271 11.7016 11.5042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20584_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20584_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:45:47.70 +00:49:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.635 3846189289977596928 146.44889896674 +00.81987793374 11.3833 10.5417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20594_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20594_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:55:32.68 +06:09:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.115 583600602857621376 133.88703233243 +06.16610556169 11.9147 11.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20596_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20596_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:23:37.41 +05:10:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.947 585507675711587200 140.90613918089 +05.18093806037 11.8637 11.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20597_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20597_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:22:31.74 +06:19:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.562 585916758460738304 140.63240641010 +06.31768116148 11.7783 11.0994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20601_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20601_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:25:46.09 +05:17:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.682 3852214922935155200 141.44222730661 +05.28445787737 12.0044 11.6000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20603_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20603_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:15:15.11 +08:25:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.248 590169085322055168 138.81302759412 +08.41932559957 12.0638 11.6742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20604_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20604_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:22:27.50 +03:29:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.084 3845650151323225344 140.61478752508 +03.49344402031 11.9520 11.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20609_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20609_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:20:00.05 +06:41:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.926 586737097214273664 140.00045239975 +06.69208041312 11.9259 11.2596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20610_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20610_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:23:45.40 +06:42:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.743 585956718836998912 140.93935079580 +06.70968182641 12.0589 11.5523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20611_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 20611_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:04:52.04 +09:25:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.812 591229323768236032 136.21705356744 +09.42005074309 12.0515 11.3491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:54.655 +05:59:02.76
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:52.549 +05:59:06.77
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:54.655 +05:59:02.76
Second-epoch second image center 09:25:52.549 +05:59:06.77
Angular distance between the image centers 0.00880 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/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.IYQrKnN1WJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.jNVl9gqkUk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.0vIIZqFrus
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.dFMK72SOW2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 5118 out of 48659 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.698635
a=0.000000 b=1.000000 c=22.698635
From vast_summary.log: estimated ref. image limiting mag.: -7.47
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 40 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
1.9 pix Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Limiting magnitude estimates:
15.2 mag. Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.2 mag. Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.1 mag. fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
15.1 mag. fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.IYQrKnN1WJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2287, passed=48648
Got 48648 stars (including 46264 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 48648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.jNVl9gqkUk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2205, passed=48320
Got 48320 stars (including 46022 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 48320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.0vIIZqFrus (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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2178, passed=43894
Got 43894 stars (including 41666 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 43894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 939 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: 0.48"
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 939 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: 0.49"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.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.dFMK72SOW2 (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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2090, passed=43214
Got 43214 stars (including 41069 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 43214 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 942 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: 0.49"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_Hya-02-Q2b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.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_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out50588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out54029.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54086.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out38235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54063.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 53336_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53336_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:58:13.57 +09:54:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 4.738 597548839863900800 134.55787321380 +09.90394748592 14.0101 13.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53345_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53345_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:56:49.13 +10:53:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.588 603873776207292928 134.20525089600 +10.89293415853 13.4901 13.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53351_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53351_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:57:57.72 +01:23:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.175 576856821303695488 134.49193355615 +01.38650094683 13.2900 12.7397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53353_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53353_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:55:42.54 +08:09:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.800 585258116635972992 133.92619360609 +08.16164402103 13.4319 12.9412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53357_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53357_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:25:32.34 +01:07:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.154 3843996765007765632 141.38507043086 +01.12199203987 13.6723 13.2287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53367_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53367_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53369_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53369_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:58:02.00 +10:57:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.633 603831307570667008 134.50898170727 +10.96613953611 13.3583 12.8176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53372_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53372_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53373_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53373_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:55:09.06 +09:47:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.357 597721153952267008 133.78864484463 +09.79383559250 12.9643 12.3268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53377_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53377_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53379_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53379_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:57:51.40 +10:18:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.505 603578664709812096 134.46543299306 +10.30568755726 13.0323 12.5276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53385_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53385_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53387_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53387_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53394_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53394_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:51:23.38 +08:27:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.374 3877976136776771968 147.84763338433 +08.45457302430 11.9054 11.3995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53483_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53483_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:45:47.71 +00:49:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.585 3846189289977596928 146.44889896674 +00.81987793374 11.3833 10.5417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53547_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53547_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53560_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53560_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 08:55:17.60 +05:58:55.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53758_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53758_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:47:46.19 +10:05:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.886 3879145609127232512 146.94298552426 +10.09554054160 13.4352 12.7544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53765_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53765_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:07:04.71 +01:26:08.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53813_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 53813_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:44:03.23 +00:48:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.321 3846198605761650432 146.01354696520 +00.81223955635 13.4618 12.9475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53833_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53833_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 53953_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 53953_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 54029_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54029_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:49:29.16 +08:15:00.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)
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Considering the candidate 54050_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54050_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:50:56.23 +09:02:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.313 3878784488276803200 147.73483658969 +09.04384324013 14.3645 13.8238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54063_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
Preparing report for the candidate 54063_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
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Considering the candidate 54073_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54073_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:56:49.54 +06:51:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.577 3850556279580177408 149.20654257215 +06.86101063819 14.0532 13.0894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54086_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54086_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:52:36.21 +09:52:55.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)
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Considering the candidate 54099_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54099_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 54106_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54106_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:17:25.71 +09:32:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 4.238 590764750041465984 139.35789745826 +09.53879679476 14.7724 14.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54112_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54112_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:56:20.30 +06:00:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.660 3850437085647828480 149.08391698645 +06.01347863707 14.6156 13.9594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54119_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54119_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:48:26.42 +06:17:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.105 3853091233702974976 147.10980359907 +06.29696313026 14.6051 14.0794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54133_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54133_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:50:27.95 +09:00:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 4.260 3878807543661262464 147.61763351441 +09.01024177200 14.3177 13.6430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54134_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54134_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:50:36.32 +09:59:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 2.105 3879175502099635072 147.65190469859 +09.99417388258 14.5528 14.0381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54138_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54138_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:11:35.60 +02:57:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.172 578770143334529408 137.89873459975 +02.95063237440 14.3783 13.6488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54159_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54159_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:35:48.92 +00:58:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.178 3841173734543577216 143.95403786741 +00.97015258617 14.5915 13.9646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54171_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54171_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:53:45.32 +09:04:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.022 3878868188599626624 148.43964410001 +09.08097017898 14.5875 13.9539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54198_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54198_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:49:28.87 +05:59:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.444 3853019941540629376 147.37017987663 +05.99586452009 14.5094 14.0271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54282_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 54282_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks
**** FOUND 09:49:02.96 +08:21:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 4.423 3854714598196799232 147.26353603205 +08.35708304022 14.6533 14.1414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50588_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051
The candidate 50588_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051 did not pass the final checks