This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1706* 03 20 08.24 +34 20 28.1 13.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.6706,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1706 13.30CV 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:08.24 +34:20:28.1 ;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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1706 2461083.6706 13.61 03:29:10.90 +31:22:05.3
158.30439 -20.45968 galactic Per Second-epoch detections are separated by 5.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:29:10.90 +31:22:05.3 (user input) | T | P | (position from user input) SpType: B:I 1980AJ.....85.1638T IRAS 03260+3111 J-Ks=3.478+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1706* 03 29 10.90 +31 22 05.3 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6706,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260212.1706 13.61CV 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:10.90 +31:22:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1706* 03 26 27.46 +25 23 08.4 13.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.6706,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1706 13.85CV 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:27.46 +25:23:08.4 ;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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1706* 02 34 57.22 +25 04 23.9 14.0 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.6706,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1706 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:34:57.22 +25:04:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1706 2461083.6706 14.29 02:54:10.80 +26:51:14.4
154.12865 -28.48048 galactic Ari Second-epoch detections are separated by 2.9" and 7.8 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 116081146261247488 | 02:54:14.18 +26:51:08.8 (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!
TCP 2026 02 12.1706* 02 54 10.80 +26 51 14.4 14.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 116081146261247488,2461083.6706,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 116081146261247488 20260212.1706 14.29CV 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:10.80 +26:51:14.4 ;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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.74422918 23.12.2025 05:51:31.401 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
First image: 2461032.74422918 23.12.2025 05:51:31.401 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Last image: 2461083.67087928 12.02.2026 04:05:53.970 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11402
Objects passed selection criteria: 11400
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: 11011.5
Average stars matched: 10826.8 (98.3222 %)
Memory usage VmPeak: 116960 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 22:14:29 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.74422918 23.12.2025 05:51:31.401 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
First image: 2461032.74422918 23.12.2025 05:51:31.401 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Last image: 2461083.67087928 12.02.2026 04:05:53.970 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 28 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): 73594
Objects passed selection criteria: 73404
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 71002.5
Average stars matched: 68794.8 (96.8906 %)
Memory usage VmPeak: 2040728 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 22:15:52 CST 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
SExtractor catalog cache: saved Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
SExtractor catalog cache: saved Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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: 2461083.67033088
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
Saving wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits to local_wcs_cache/
'wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits' -> 'local_wcs_cache/wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits'
wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits exists and is non-empty
Saving wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits to local_wcs_cache/
'wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits' -> 'local_wcs_cache/wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits'
wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
Saving wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits'
wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits exists and is non-empty
Saving wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits to local_wcs_cache/
'wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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 03:00:00.362 +29:59:53.96
Second-epoch image center 02:59:59.441 +30:00:08.32
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 03:00:00.362 +29:59:53.96
Second-epoch image center 03:00:02.333 +30:00:39.15
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 02:59:59.441 +30:00:08.32
Second-epoch second image center 03:00:02.333 +30:00:39.15
Angular distance between the image centers 0.01350 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.yrpUnGhTv6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits &> /tmp/tmp.EpYGAWYT45
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.wWyesMqHHN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.ymhAbVLra4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
Found non-empty wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
The reference image (wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits) and catalog (wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat) found
'wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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 5689 out of 11919 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.944362
a=0.000000 b=1.000000 c=22.944362
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
2.1 pix Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
2.1 pix fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Limiting magnitude estimates:
15.4 mag. Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
15.4 mag. Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
15.2 mag. fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
15.2 mag. fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.yrpUnGhTv6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=912, passed=11919
Got 11919 stars (including 10998 good ones) from the SExtractor catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 11919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.32"
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 961 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 - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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.EpYGAWYT45 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits' -> 'wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS-calibrated image found: wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
Checking if the catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS catalog name: wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=882, passed=11826
Got 11826 stars (including 10927 good ones) from the SExtractor catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat
util/solve_plate_with_UCAC5 got 11826 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits -region wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.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.wWyesMqHHN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=757, passed=10278
Got 10278 stars (including 9512 good ones) from the SExtractor catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat
util/solve_plate_with_UCAC5 got 10278 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
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_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.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.ymhAbVLra4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=758, passed=10277
Got 10277 stars (including 9507 good ones) from the SExtractor catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 10277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits'
Saving fully-calibrated image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits'
Preparing the HTML report for the field Ari-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20654_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 20654_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:11:17.18 +34:50:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20658_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 20658_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:14:39.53 +33:18:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20670_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 20670_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:50:04.84 +29:07:51.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Ari-01-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
SExtractor catalog cache: saved Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat to cache
SExtractor catalog cache: saved Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Creating symlink local_wcs_cache/wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits exists and is non-empty
wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits exists and is non-empty
wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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 03:00:00.362 +29:59:53.96
Second-epoch image center 02:59:59.441 +30:00:08.32
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 03:00:00.362 +29:59:53.96
Second-epoch image center 03:00:02.333 +30:00:39.15
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 02:59:59.441 +30:00:08.32
Second-epoch second image center 03:00:02.333 +30:00:39.15
Angular distance between the image centers 0.01350 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits &> /tmp/tmp.XH7dBuclNm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits &> /tmp/tmp.0IRAj62u1F
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.6Fm2nY18yy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.8MKXgIjbeY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
Found non-empty wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits and wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
The reference image (wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits) and catalog (wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat) found
'wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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 5747 out of 74872 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.814421
a=0.000000 b=1.000000 c=22.814421
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
1.9 pix Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
1.9 pix fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Limiting magnitude estimates:
15.6 mag. Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
15.6 mag. Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
15.4 mag. fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
15.4 mag. fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XH7dBuclNm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits' -> 'wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS_IMAGE_NAME=wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS-calibrated image found: wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
Checking if the catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits alredy exist and is non-empty...
Catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits
WCS catalog name: wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=4792, passed=74858
Got 74858 stars (including 69948 good ones) from the SExtractor catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat
util/solve_plate_with_UCAC5 got 74858 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits -region wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.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.0IRAj62u1F (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits' -> 'wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS-calibrated image found: wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
Checking if the catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat corresponding to the image wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits
WCS catalog name: wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=4834, passed=75250
Got 75250 stars (including 70272 good ones) from the SExtractor catalog wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat
util/solve_plate_with_UCAC5 got 75250 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits -region wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-01-Q1b1x1_2025-12-22_23-52-16_20.00sec_-15.00C_LIGHT_0269.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.6Fm2nY18yy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=3950, passed=68105
Got 68105 stars (including 64029 good ones) from the SExtractor catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat
util/solve_plate_with_UCAC5 got 68105 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.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.8MKXgIjbeY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=3866, passed=67552
Got 67552 stars (including 63553 good ones) from the SExtractor catalog wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 67552 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 962 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.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_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-06_20.00sec_-15.00C_LIGHT_0131.fits
Saving fully-calibrated image wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.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_2026-02-11_CI_Ari-01-Q1b1x1_221212_TTUQ1b1x1_1051_uUM7MkLR/wcs_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132.fits
Preparing the HTML report for the field Ari-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out90978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out91038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91134.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 90978_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 90978_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:45:48.48 +27:03:05.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
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Considering the candidate 91019_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91019_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:46:45.29 +34:50:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.381 140122384615756160 041.68861738430 +34.83606403668 12.7603 12.0704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91034_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91034_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:46:47.20 +34:50:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.562 140122384615756288 041.69681691239 +34.83359580467 13.2497 12.8096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91038_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
Preparing report for the candidate 91038_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
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Considering the candidate 91048_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91048_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:27:19.63 +32:43:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91055_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91055_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:00:27.50 +33:38:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91056_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
Preparing report for the candidate 91056_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
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Considering the candidate 91062_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91062_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:42:23.56 +33:36:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91070_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91070_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:27:39.33 +33:13:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.354 124858929839634432 051.91309554445 +33.22532712169 13.9529 13.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91075_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91075_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:01:03.55 +28:14:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.137 116647295968365312 045.26443418137 +28.23850594360 13.7096 13.1094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91077_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91077_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:24:20.78 +24:45:13.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91079_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
Preparing report for the candidate 91079_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
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Considering the candidate 91086_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91086_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:49:58.42 +25:44:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.914 114494898875295616 042.49355836801 +25.73964160253 13.9299 13.1859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91091_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91091_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:12:56.56 +29:16:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.226 122068163169188352 048.23533745305 +29.27876141849 14.1127 13.4668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91104_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
Preparing report for the candidate 91104_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
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Considering the candidate 91105_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91105_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:25:08.02 +33:35:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91115_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91115_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:50:10.67 +35:00:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.348 140095790178326528 042.54400628229 +35.00663893720 14.0814 13.5889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91116_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91116_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:51:50.58 +33:07:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91118_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91118_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:42:10.84 +30:54:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91119_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91119_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:19:42.74 +27:32:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91134_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
Preparing report for the candidate 91134_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
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Considering the candidate 91140_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91140_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:24:12.06 +31:50:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.692 132697348232734208 036.05011403764 +31.84123538644 14.5839 14.0380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91150_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91150_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:02:28.34 +27:52:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91151_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91151_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:45:05.51 +32:42:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91156_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91156_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:09:31.62 +26:42:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.239 112550412562657536 047.38197315620 +26.70400261218 14.5759 13.8378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91162_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91162_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:00:06.90 +33:12:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.438 136823471775297792 045.02827259814 +33.20560792412 14.3581 13.7465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91170_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91170_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:29:44.45 +33:43:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.127 124899543050241792 052.43484505283 +33.72330741440 14.4791 13.7658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91171_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91171_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:58:49.93 +32:40:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)
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Considering the candidate 91180_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91180_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:24:37.58 +33:42:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91195_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91195_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:41:43.81 +34:01:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91202_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91202_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:47:00.95 +32:06:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.049 130555499582680960 041.75428152735 +32.11242758001 14.6498 14.0916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91217_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91217_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:38:36.14 +26:20:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.335 126536097387545600 039.65054125568 +26.34397408197 14.5837 14.0192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91234_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 91234_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:31:14.63 +33:07:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.480 134423787648150144 037.80989715483 +33.11881405751 14.6822 13.9476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16643_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132
The candidate 16643_fd_Ari-01-Q1b1x1_2026-02-11_22-05-53_20.00sec_-15.00C_LIGHT_0132 did not pass the final checks