This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt
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
VARIABLE_NAME,2461098.7244,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2244 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:39.76 +02:28:02.0 ;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-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_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
TU Hya,2461098.7244,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TU Hya 20260227.2244 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:58:16.60 -00:49:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_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
WW Hya,2461098.7244,10.65,0.05,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
WW Hya 20260227.2244 10.65CV 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:46.82 -03:16:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_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 02 27.2244* 09 54 08.67 +02 00 26.3 13.9 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
VARIABLE_NAME,2461098.7244,13.86,0.05,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 20260227.2244 13.86CV 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:08.67 +02:00:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_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 02 27.2244* 09 44 15.02 +02 09 54.3 14.0 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
VARIABLE_NAME,2461098.7244,13.98,0.05,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 20260227.2244 13.98CV 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:44:15.02 +02:09:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2244 2461098.7244 13.97 09:53:40.21 +01:34:48.1
236.19445 40.37199 galactic Sex Second-epoch detections are separated by 8.0" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:53:40.21 +01:34:48.1 (user input) | T | P | (position from user input) J-Ks=13.260+/- (unrealisitic color!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2244* 09 53 40.21 +01 34 48.1 14.0 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,2461098.7244,13.97,0.05,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 20260227.2244 13.97CV 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:40.21 +01:34:48.1 ;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-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_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
RZ Hya,2461098.7244,11.88,0.05,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
RZ Hya 20260227.2244 11.88CV 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:24:50.29 -06:47:31.1 ;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-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461098.72464081 27.02.2026 05:23:18.966 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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): 9915
Objects passed selection criteria: 9894
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 8393
Average stars matched: 8247.75 (98.2694 %)
Memory usage VmPeak: 115780 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 02:18:55 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461098.72464081 27.02.2026 05:23:18.966 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 23 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): 59986
Objects passed selection criteria: 59870
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 52327.8
Average stars matched: 50597.5 (96.6934 %)
Memory usage VmPeak: 160028 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 02:20:47 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Hya-04-Q2b1x1
#######################################
########### Starting Hya-04-Q2b1x1 ###########
Processing Hya-04-Q2b1x1
server tau has sufficient free disk space available: 747437 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 747437 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.png' -> 'transient_report/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits_preview.png'
Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
renamed 'Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.png' -> 'transient_report/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits_preview.png'
Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 740.6366
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 593.7101
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 2302.3953
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 705.7045
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 2299.5032
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 704.8486
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 3.10867
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461098.72409839
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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits'
wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:43.539 -01:59:40.17
Angular distance between the image centers 0.01 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:45.122 -02:00:00.51
Angular distance between the image centers 0.01 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 09:25:43.539 -01:59:40.17
Second-epoch second image center 09:25:45.122 -02:00:00.51
Angular distance between the image centers 0.00868 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.RkUJuKC9yo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.5RS1jE1ohe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits &> /tmp/tmp.clt71qG7nR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits &> /tmp/tmp.tBcb2oDvfT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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 5565 out of 10420 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.932573
a=0.000000 b=1.000000 c=22.932573
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
2.0 pix Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
2.4 pix Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
2.4 pix Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Limiting magnitude estimates:
15.3 mag. Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.3 mag. Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
14.5 mag. Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
14.5 mag. Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.RkUJuKC9yo (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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=740, passed=10420
Got 10420 stars (including 9668 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 10420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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: 0.27"
Estimated accuracy of the plate solution: 0.26"
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_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.5RS1jE1ohe (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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=743, passed=10444
Got 10444 stars (including 9684 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 10444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 936 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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.clt71qG7nR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=6475
Got 6475 stars (including 5773 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 6475 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 945 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits -region wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.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.tBcb2oDvfT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=718, passed=6491
Got 6491 stars (including 5767 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 6491 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits -region wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Hya-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20544.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20544_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 20544_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20550_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 20550_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:24:50.30 -06:47:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.295 5745316492741496320 141.20975797736 -06.79280804443 10.4424 8.8635 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06636_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 06636_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04227_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 04227_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Hya-04-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 ####
08:57:46.82 -03:16:53.7
08:58:16.60 -00:49:53.3
09:03:39.76 +02:28:02.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits exists and is non-empty
wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:43.539 -01:59:40.17
Angular distance between the image centers 0.01 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:45.122 -02:00:00.51
Angular distance between the image centers 0.01 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 09:25:43.539 -01:59:40.17
Second-epoch second image center 09:25:45.122 -02:00:00.51
Angular distance between the image centers 0.00868 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.SohPrmQsLe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.n9jXGjEaGb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits &> /tmp/tmp.erC4GpuN68
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits &> /tmp/tmp.2UXEsajMox
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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 5627 out of 64348 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.821408
a=0.000000 b=1.000000 c=22.821408
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
1.9 pix Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
2.2 pix Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
2.2 pix Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Limiting magnitude estimates:
15.4 mag. Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.4 mag. Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
14.7 mag. Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
14.7 mag. Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.SohPrmQsLe (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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=3271, passed=64335
Got 64335 stars (including 60948 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 64335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.n9jXGjEaGb (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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3228, passed=64125
Got 64125 stars (including 60786 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 64125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 943 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.erC4GpuN68 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2143, passed=41252
Got 41252 stars (including 39054 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 41252 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 948 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits -region wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-22-32_20.00sec_-15.00C_LIGHT_0064.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.2UXEsajMox (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2136, passed=41237
Got 41237 stars (including 39035 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 41237 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q2b1x1_232744_TTUQ2b1x1_8063_w5r5mtWt/Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits -region wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Hya-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out31504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79552.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 78818_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78818_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:58:59.76 -06:25:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.218 5757389027335494784 134.74839456629 -06.42858950152 14.1678 13.6779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78830_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78830_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:55:23.67 +02:26:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.506 3846829450558142976 148.84828328907 +02.43745258305 13.6186 13.1860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78834_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78834_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:59:14.18 -06:19:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.318 5757414281743186432 134.80900252460 -06.31933334342 13.7178 13.1548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78835_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78835_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:11:12.99 +01:27:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.061 3843690104342772608 137.80461147224 +01.45371917424 12.7473 11.5339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78840_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78840_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:37:07.27 -04:41:17.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 78844_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78844_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:09:02.81 +01:04:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.110 3843593858420051584 137.26226624295 +01.07609674503 12.7209 11.6422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78845_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78845_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:49:05.85 -04:41:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.704 3822774571388874368 147.27424657112 -04.69518315840 13.7797 13.3428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78848_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78848_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:48:22.74 -00:05:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.573 3834024572500807296 147.09460762994 -00.09506794739 13.7631 13.2440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78849_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78849_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:48:20.66 -06:15:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.166 3820896334945850496 147.08582145967 -06.25616818072 13.5410 13.0592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78854_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78854_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:57:13.49 -06:09:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.937 5757599132840546816 134.30603502806 -06.15544386832 12.3560 11.8289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78856_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78856_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:36:24.94 +02:47:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.305 3847614948536955136 144.10327723896 +02.78421268900 12.9169 12.4349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78858_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78858_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:47:07.62 +02:45:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.713 3847048768768158464 146.78160283156 +02.75679922655 12.3557 11.8142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78909_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 78909_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:03:39.76 +02:28:01.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 79019_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79019_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:35:52.74 -05:22:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.229 3824025918699997952 143.96943391845 -05.37789548991 12.7062 12.2872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79025_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79025_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:55:36.24 +00:10:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.399 3834269759298349952 148.90061158043 +00.16945161759 12.2268 11.8114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79031_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79031_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:26:15.03 -01:28:52.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79047_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79047_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:51:09.22 -00:50:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.289 3833705679769232640 147.78849669915 -00.84945182468 12.6588 12.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79057_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79057_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:44:13.38 +01:49:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.272 3846582331024583424 146.05541971426 +01.82382056862 12.5206 11.9332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79063_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79063_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:29:10.70 -02:48:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.422 3837697555519034368 142.29446946417 -02.80488996785 12.8974 12.2836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79080_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79080_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:52:17.08 +00:05:38.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79150_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79150_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:39:41.83 -04:56:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.116 3824253659341617664 144.92401171672 -04.94472596154 13.4325 12.9657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79214_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79214_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:26:18.19 -04:43:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.428 3825020568702088576 141.57485709040 -04.72094107586 13.6807 13.1657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79257_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79257_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:55:15.93 -03:56:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.601 3823117756455375104 148.81603783208 -03.94354242388 13.1353 12.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79260_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79260_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:18:11.60 -07:03:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.900 5745706750649918208 139.54796983118 -07.06105917306 13.6536 13.2344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79279_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79279_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:37:06.63 -01:54:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.697 3827350468200705920 144.27704903010 -01.90954849349 13.8031 13.2725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79299_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79299_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:44:50.66 -00:37:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.144 3828000863687903488 146.21054224061 -00.62791807308 14.4606 13.6864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79300_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79300_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:50:18.84 -03:51:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.140 3822979600242817536 147.57768632554 -03.85240351555 13.8152 13.4123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79305_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79305_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:47:17.24 +02:39:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.243 3847044954837200128 146.82164335772 +02.66628847494 13.5957 13.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79342_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79342_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:34:17.56 -07:03:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.150 3823558836712429440 143.57328916895 -07.06368428650 13.7880 13.2313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79359_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79359_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:40:22.52 -02:35:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.040 3827149566810584320 145.09354927803 -02.58644574234 14.0789 13.5128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79360_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79360_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:37:51.78 -03:24:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.409 3825452642411975936 144.46508032192 -03.41247154640 14.2398 13.7506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79376_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79376_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:08:29.52 -05:38:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.318 5758265750419525760 137.12304478739 -05.64688169645 13.7348 13.2908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79438_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79438_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:48:13.69 -04:27:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.507 3822832093886037632 147.05728161593 -04.45740641084 13.8667 13.3832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79478_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 79478_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
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Considering the candidate 79488_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79488_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:45:27.42 -05:42:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.642 3821176985288793472 146.36353581807 -05.70195608425 14.3426 13.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79493_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 79493_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
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Considering the candidate 79552_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 79552_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
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Considering the candidate 79628_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79628_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:44:27.55 -02:13:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.779 3827502716201538688 146.11449741179 -02.21713049956 14.4261 13.9460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79697_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 79697_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:45:12.05 -04:29:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.333 3825822284477253248 146.30007078433 -04.48714436619 14.4851 13.9853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25919_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 25919_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:57:46.84 -03:16:53.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52576_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 52576_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:58:16.61 -00:49:53.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 31504_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 31504_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks
**** FOUND 09:34:14.21 -02:25:04.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 03064_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
Preparing report for the candidate 03064_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
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Considering the candidate 14335_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065
The candidate 14335_Hya-04-Q2b1x1_2026-02-26_23-23-18_20.00sec_-14.90C_LIGHT_0065 did not pass the final checks