This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 13.23 11:05:39.00 -30:34:33.0
277.44045 27.00721 galactic Hya Second-epoch detections are separated by 0.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:05:39.00 -30:34:33.0 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6560,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1560 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:39.00 -30:34:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.99 11:05:35.22 -30:24:02.4
277.33919 27.15800 galactic Hya Second-epoch detections are separated by 3.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5452473905831060480 | 11:05:35.72 -30:24:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5452473905831060480,2461119.6560,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5452473905831060480 20260320.1560 12.99CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:35.22 -30:24:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 13.03 11:08:21.44 -29:24:07.2
277.44803 28.31925 galactic Hya Second-epoch detections are separated by 2.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5452673123594011648 | 11:08:20.47 -29:24:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5452673123594011648,2461119.6560,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5452673123594011648 20260320.1560 13.03CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:08:21.44 -29:24:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.96 11:07:01.14 -29:59:20.4
277.44565 27.66424 galactic Hya Second-epoch detections are separated by 3.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5452509880477250944 | 11:07:00.32 -29:59:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5452509880477250944,2461119.6560,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5452509880477250944 20260320.1560 12.96CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:01.14 -29:59:20.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5452479678267203840,2461119.6560,12.86,0.05,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
Gaia DR3 5452479678267203840 20260320.1560 12.86CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:06:22.78 -30:14:20.1 ;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-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.62 11:05:29.79 -29:34:11.0
276.90021 27.89238 galactic Hya Second-epoch detections are separated by 0.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5453332109016133376 | 11:05:29.09 -29:34:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5453332109016133376,2461119.6560,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5453332109016133376 20260320.1560 12.62CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:29.79 -29:34:11.0 ;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-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 13.03 11:03:45.82 -29:28:37.7
276.47262 27.80445 galactic Hya Second-epoch detections are separated by 1.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5453329188438231936 | 11:03:45.35 -29:28:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5453329188438231936,2461119.6560,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5453329188438231936 20260320.1560 13.03CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:45.82 -29:28:37.7 ;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-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.62 11:05:42.67 -29:13:12.8
276.76958 28.22562 galactic Hya Second-epoch detections are separated by 5.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J166.4255-29.2201 | 11:05:42.12 -29:13:12.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J166.4255-29.2201,2461119.6560,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J166.4255-29.2201 20260320.1560 12.62CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:42.67 -29:13:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.81 10:57:11.02 -30:02:07.2
275.34392 26.64526 galactic Hya Second-epoch detections are separated by 7.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5453063656380630528 | 10:57:12.86 -30:02:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5453063656380630528,2461119.6560,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5453063656380630528 20260320.1560 12.81CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:57:11.02 -30:02:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1560 2461119.6560 12.74 11:04:19.68 -30:12:47.2
276.97162 27.20384 galactic Hya Second-epoch detections are separated by 2.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5452152504838427264 | 11:04:20.19 -30:12:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5452152504838427264,2461119.6560,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5452152504838427264 20260320.1560 12.74CV 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:19.68 -30:12:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20_00sec_-14_90C_LIGHT_0114_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: 2461061.87457016 21.01.2026 08:59:12.862 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
First image: 2461061.87457016 21.01.2026 08:59:12.862 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Last image: 2461119.65627331 20.03.2026 03:44:52.014 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.11
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: 4 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): 7809
Objects passed selection criteria: 7805
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7497.25
Average stars matched: 7374.5 (98.3627 %)
Memory usage VmPeak: 113852 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 22:52:03 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.87457016 21.01.2026 08:59:12.862 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
First image: 2461061.87457016 21.01.2026 08:59:12.862 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Last image: 2461119.65627331 20.03.2026 03:44:52.014 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.81
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: 18 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): 52561
Objects passed selection criteria: 52458
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 48645
Average stars matched: 47263.5 (97.16 %)
Memory usage VmPeak: 153524 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 22:53:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.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: 2461119.65567321
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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits'
wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:41.203 -25:59:42.45
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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:38.147 -25:59:22.73
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 10:33:41.203 -25:59:42.45
Second-epoch second image center 10:33:38.147 -25:59:22.73
Angular distance between the image centers 0.01269 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.vYE1t4yBeJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits &> /tmp/tmp.CyMLoRtvwJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.jgVG7hQZrp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.ve9h89QGKy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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 6213 out of 8052 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.818360
a=0.000000 b=1.000000 c=22.818360
From vast_summary.log: estimated ref. image limiting mag.: -8.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.71
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.71
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
2.0 pix Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
2.5 pix fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
2.5 pix fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Limiting magnitude estimates:
14.7 mag. Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
14.7 mag. Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
14.3 mag. fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
14.3 mag. fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (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.vYE1t4yBeJ (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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=581, passed=8052
Got 8052 stars (including 7465 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 8052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 963 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 - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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.CyMLoRtvwJ (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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=565, passed=8068
Got 8068 stars (including 7487 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 8068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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.jgVG7hQZrp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=394, passed=6995
Got 6995 stars (including 6598 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat
util/solve_plate_with_UCAC5 got 6995 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 960 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.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.ve9h89QGKy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=411, passed=7040
Got 7040 stars (including 6621 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 7040 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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits'
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits'
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20442.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20435_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20435_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:18:33.97 -25:19:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.451 5472330364272060800 154.64183126314 -25.33005648737 11.4109 10.9650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20437_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20437_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:47:43.72 -25:35:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.753 5470197277356005888 161.93211328260 -25.59304655641 10.8639 9.6747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20439_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20439_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:19:01.40 -24:30:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.407 5473564909673449344 154.75594784534 -24.50154382185 11.4899 10.8807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20440_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20440_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:33:04.70 -26:32:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 0.946 5469200222171475968 158.26979274788 -26.54167703521 11.5253 10.8356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20441_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20441_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:23:30.79 -26:26:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.892 5469017982415855104 155.87856731576 -26.43728501015 11.6426 10.9463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20442_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 20442_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:33:37.76 -25:24:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.915 5470835784373783936 158.40760354362 -25.40745934571 11.6745 11.2168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:41.203 -25:59:42.45
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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:38.147 -25:59:22.73
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 10:33:41.203 -25:59:42.45
Second-epoch second image center 10:33:38.147 -25:59:22.73
Angular distance between the image centers 0.01269 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.8GqEZxSC3U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits &> /tmp/tmp.QaKRV3FTX2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.faqV8kjkrv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.ilY2SQVHuw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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 7312 out of 56496 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.651562
a=0.000000 b=1.000000 c=22.651562
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 64 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
1.9 pix Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
2.4 pix fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
2.4 pix fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Limiting magnitude estimates:
14.8 mag. Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
14.8 mag. Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
14.4 mag. fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
14.4 mag. fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (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.8GqEZxSC3U (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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2594, passed=56489
Got 56489 stars (including 53792 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 56489 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 965 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: 0.30"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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.QaKRV3FTX2 (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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2585, passed=55964
Got 55964 stars (including 53278 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 55964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 963 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: 0.28"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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.faqV8kjkrv (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1901, passed=41754
Got 41754 stars (including 39802 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat
util/solve_plate_with_UCAC5 got 41754 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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.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.ilY2SQVHuw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1923, passed=41734
Got 41734 stars (including 39761 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 41734 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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-00_20.00sec_-14.90C_LIGHT_0114.fits
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-10-Q2b1x1_224949_TTUQ2b1x1_23548_cOEQJ0Zs/wcs_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115.fits
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out66522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out70807.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out70786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70829.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 70752_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70752_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:14:07.39 -24:05:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.457 5473463204848218880 153.53037636312 -24.09130291377 14.3621 13.7346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70761_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70761_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:34:08.62 -29:43:56.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 70765_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70765_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:06:34.86 -24:23:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.270 3536282802295273088 166.64475797618 -24.39428998715 13.2606 12.6869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70768_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70768_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 70770_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70770_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:00:51.18 -30:13:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.134 5452902303048748928 165.21262515519 -30.22903306315 12.7045 12.1401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70774_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70774_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 70775_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70775_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:10:12.69 -20:47:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70778_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70778_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:07:09.21 -29:54:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.465 5452512487520438400 166.78727190298 -29.90025248557 12.5155 11.9085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70786_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70786_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70787_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70787_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:03:39.77 -29:43:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.061 5453304140189023872 165.91588144528 -29.73299650975 12.4376 11.9839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70788_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70788_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:04:59.52 -29:00:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.705 5453366365675182080 166.24741133793 -29.01409146990 12.5392 12.0947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70791_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70791_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:07:24.01 -28:21:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.247 5453552320579283200 166.84944406101 -28.35284369516 12.4262 11.8228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70793_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70793_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:00:13.62 -29:53:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.747 5463773930427022720 150.05716752302 -29.89462112209 13.1542 12.7409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70794_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70794_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:02:50.93 -30:03:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.478 5452919551637560576 165.71340054332 -30.06124982380 12.1139 11.6435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70797_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70797_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:06:15.74 -30:52:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.818 5451885319215384448 166.56434784375 -30.87188713445 12.1726 11.6565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70800_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70800_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70801_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70801_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70803_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70803_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70804_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70804_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:19:39.06 -21:57:18.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 70805_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70805_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:05:04.83 -27:35:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.957 3532300130661243904 166.27065074833 -27.58508116033 12.3800 12.0011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70807_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70807_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:03:03.02 -30:11:02.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 70808_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70808_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70809_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70809_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:07:15.84 -27:35:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 3.549 3532244978984251520 166.81696545459 -27.59398255799 12.2390 11.7799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70811_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70811_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 70813_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70813_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:03:38.71 -30:39:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.415 5452135393688687616 165.91056701114 -30.65533565218 12.1134 11.5192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70814_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70814_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:06:23.42 -27:27:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.650 3532260926199862272 166.59713141415 -27.45861743396 12.0900 11.4605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70815_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70815_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 70818_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70818_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:03:22.05 -29:56:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.593 5452922227399871488 165.84043044951 -29.94485818323 12.1522 11.6441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70819_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70819_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70820_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70820_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 70821_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70821_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70823_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70823_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70824_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70824_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:49:09.67 -22:11:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70826_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70826_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70827_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70827_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 70829_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
Preparing report for the candidate 70829_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
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Considering the candidate 70830_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70830_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:05:25.74 -30:47:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.119 5452072034331287680 166.35689794454 -30.78844954770 11.7055 10.8945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70833_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70833_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:08:21.35 -30:30:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 5.012 5452270938559727104 167.08734261901 -30.50024105153 11.7816 11.3306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70837_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70837_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:06:42.61 -29:31:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 4.332 5452585540621001088 166.67618500393 -29.51948324582 11.7814 11.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70839_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70839_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 70841_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70841_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:07:03.01 -30:32:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.776 5452454595658255616 166.76275664893 -30.54011049626 11.5642 10.8720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70842_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70842_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 70843_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70843_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 70849_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70849_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 70850_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70850_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:06:41.66 -30:16:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 4.003 5452479025432176256 166.67485223519 -30.26686764400 10.9595 10.5041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70853_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70853_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 70854_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70854_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 11:07:22.28 -28:59:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.827 5453449310083754752 166.84160233785 -28.98881216307 10.7868 10.2503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70855_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70855_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 70856_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70856_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 70888_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70888_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:16:14.62 -21:00:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70943_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 70943_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:11:56.13 -21:16:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.028 5666612797590396800 152.98417879417 -21.26679694019 13.0531 12.6106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71017_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71017_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:24:12.54 -27:24:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.837 5468633256425286656 156.05226296006 -27.40971203829 13.8881 13.2620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71023_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71023_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:28:42.77 -23:46:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.729 5474225887960262272 157.17783140502 -23.78206014296 14.1237 13.6411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71056_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71056_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:09:08.60 -23:28:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.721 5665742946454354560 152.28548989913 -23.47631020888 13.9178 13.3752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71067_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71067_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:13:53.56 -21:48:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.169 5666522534557845760 153.47325324046 -21.81695997778 14.1157 13.6123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71131_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71131_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:46:29.45 -21:08:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.202 3550508489893538688 161.62306641833 -21.14336313178 14.4312 13.9526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71140_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71140_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 71156_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71156_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:50:24.01 -21:16:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.947 3550621670871484032 162.60004586298 -21.27684623735 14.4352 13.9338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71183_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71183_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:40:40.11 -21:07:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 0.978 3553464286386704768 160.16712216431 -21.12022847946 14.5399 14.0746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71193_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71193_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:43:42.50 -21:32:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.521 3550381874257455744 160.92714511578 -21.54003387455 14.4288 13.8035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71203_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71203_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:31:47.73 -24:30:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.559 5471128288826720000 157.94812993039 -24.50152495183 14.6468 14.0790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71207_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71207_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:40:37.08 -23:27:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.683 5471636194479494656 160.15413438911 -23.45179786599 14.6776 14.1058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71210_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 71210_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:32:44.51 -23:10:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.212 5474373772274139136 158.18551853065 -23.17802008706 14.5730 14.0853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66522_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115
The candidate 66522_fd_Hya-10-Q2b1x1_2026-03-19_22-44-52_20.00sec_-15.00C_LIGHT_0115 did not pass the final checks