This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw
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 22.1634* 05 09 05.14 -02 39 40.6 13.6 U Ori 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,2461093.6634,13.57,0.05,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 20260222.1634 13.57CV 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:05.14 -02:39:40.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1634 2461093.6634 13.99 05:19:15.70 -02:04:53.0
203.90769 -21.38956 galactic Ori Second-epoch detections are separated by 1.4" and 2.6 pix This object is listed in tocp_transients_list.txt 4.7" TCP J05191540-0204515 2026-02-13.4306 14.5mag
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.8146-02.0813 | 05:19:15.70 -02:04:53.0 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: em 1991PASJ...43...27W Kiso A-0975 46
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 22.1634* 05 19 15.70 -02 04 53.0 14.0 U Ori 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
ATO J079.8146-02.0813,2461093.6634,13.99,0.05,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
ATO J079.8146-02.0813 20260222.1634 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:15.70 -02:04:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_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 22.1634* 05 23 51.97 +01 00 31.0 14.4 U Ori 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
BI Ori,2461093.6634,14.38,0.05,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
BI Ori 20260222.1634 14.38CV 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:51.97 +01:00:31.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_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 22.1634* 05 10 58.16 -01 20 28.5 14.5 U Ori 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,2461093.6634,14.48,0.05,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 20260222.1634 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:58.16 -01:20:28.5 ;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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_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 22.1634* 05 36 00.29 -06 42 33.8 13.4 U Ori 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
AV Ori,2461093.6634,13.39,0.05,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
AV Ori 20260222.1634 13.39CV 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:00.29 -06:42:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_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 22.1634* 05 38 33.82 -02 44 14.2 12.4 U Ori 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
TX Ori,2461093.6634,12.38,0.05,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
TX Ori 20260222.1634 12.38CV 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:33.82 -02:44:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1634 2461093.6634 12.69 04:39:30.11 -04:36:01.7
201.04119 -31.30048 galactic Eri Second-epoch detections are separated by 0.4" and 2.6 pix This object is listed in neverexclude_list.txt 3.7" BF Eri - AAVSO HST campaignThe object was found in VSX 4" BF Eri
Type: UG
# Max. Min./Amp. JD0 Period
12.300 V 15.200 V 0.270880400000 K3
The object was not found in astcheck.
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 22.1634* 04 39 30.11 -04 36 01.7 12.7 U Eri 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
BF Eri,2461093.6634,12.69,0.05,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
BF Eri 20260222.1634 12.69CV 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:30.11 -04:36:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20_00sec_-15_00C_LIGHT_0301_fits__*pix.png resample_wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20_00sec_-15_00C_LIGHT_0118_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: 2461032.76284740 23.12.2025 06:18:20.015 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
First image: 2461032.76284740 23.12.2025 06:18:20.015 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Last image: 2461093.66365227 22.02.2026 03:55:29.556 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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: 6 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): 14382
Objects passed selection criteria: 14375
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: 13908.5
Average stars matched: 13656.8 (98.19 %)
Memory usage VmPeak: 119296 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 Sat Feb 21 22:03:22 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: 2461032.76284740 23.12.2025 06:18:20.015 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
First image: 2461032.76284740 23.12.2025 06:18:20.015 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Last image: 2461093.66365227 22.02.2026 03:55:29.556 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 215
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 50 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): 87579
Objects passed selection criteria: 87381
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: 84237
Average stars matched: 81670 (96.9526 %)
Memory usage VmPeak: 1882452 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 Sat Feb 21 22:05:25 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat to cache
SExtractor catalog cache: saved Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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: 2461093.66323216
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits exists and is non-empty
Saving wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits to local_wcs_cache/
'wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits exists and is non-empty
Saving wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits to local_wcs_cache/
'wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits' -> 'local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits'
wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits'
wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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 05:08:15.177 -01:59:04.10
Second-epoch image center 05:08:34.934 -02:00:04.21
Angular distance between the image centers 0.08 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 05:08:15.177 -01:59:04.10
Second-epoch image center 05:08:34.518 -01:59:50.20
Angular distance between the image centers 0.08 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 05:08:34.934 -02:00:04.21
Second-epoch second image center 05:08:34.518 -01:59:50.20
Angular distance between the image centers 0.00426 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits &> /tmp/tmp.SI1dM2itAx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits &> /tmp/tmp.ZUzDa4KPSc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits &> /tmp/tmp.g6axEuB2X2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.DW58AWh1hH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
The reference image (wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits) and catalog (wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat) found
'wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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 8007 out of 14808 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.921444
a=0.000000 b=1.000000 c=22.921444
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
2.0 pix Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
2.1 pix fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
2.1 pix fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.2 mag. Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
15.2 mag. Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
15.0 mag. fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
15.1 mag. fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SI1dM2itAx (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> 'wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Checking if the catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS catalog name: wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1520, passed=14808
Got 14808 stars (including 13268 good ones) from the SExtractor catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 14808 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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 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: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits -region wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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.ZUzDa4KPSc (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits' -> 'wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS-calibrated image found: wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
Checking if the catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS catalog name: wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1525, passed=14761
Got 14761 stars (including 13221 good ones) from the SExtractor catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat
util/solve_plate_with_UCAC5 got 14761 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 947 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits -region wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.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.g6axEuB2X2 (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1398, passed=13283
Got 13283 stars (including 11874 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 13283 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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits -region wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.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.DW58AWh1hH (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1429, passed=13160
Got 13160 stars (including 11717 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 13160 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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits'
Saving fully-calibrated image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits'
Preparing the HTML report for the field Ori-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20870.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20812_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 20812_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:37:37.19 +02:19:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20859_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 20859_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:16:35.94 +00:25:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20864_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 20864_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:10:25.65 -00:12:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20870_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 20870_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:36:09.72 -05:27:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.891 3017348803299280896 084.04025156617 -05.46422796479 12.5176 11.9785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11561_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 11561_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:29:00.56 -04:41:32.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Ori-05-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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat to cache
SExtractor catalog cache: saved Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Creating symlink local_wcs_cache/wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits exists and is non-empty
wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits exists and is non-empty
wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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 05:08:15.177 -01:59:04.10
Second-epoch image center 05:08:34.934 -02:00:04.21
Angular distance between the image centers 0.08 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 05:08:15.177 -01:59:04.10
Second-epoch image center 05:08:34.518 -01:59:50.20
Angular distance between the image centers 0.08 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 05:08:34.934 -02:00:04.21
Second-epoch second image center 05:08:34.518 -01:59:50.20
Angular distance between the image centers 0.00426 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/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits &> /tmp/tmp.aK5QpYNLuW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits &> /tmp/tmp.UognoZAPXd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits &> /tmp/tmp.FwYGdd276Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.odz1yGDbzr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
Found non-empty wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits and wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
The reference image (wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits) and catalog (wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat) found
'wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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 8144 out of 88569 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.802433
a=0.000000 b=1.000000 c=22.802433
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 83 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
1.9 pix Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
2.0 pix fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
1.9 pix fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.4 mag. Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
15.4 mag. Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
15.2 mag. fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
15.2 mag. fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (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.aK5QpYNLuW (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits' -> 'wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
Checking if the catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits
WCS catalog name: wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=7123, passed=88536
Got 88536 stars (including 81282 good ones) from the SExtractor catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 88536 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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 948 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: 0.36"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits -region wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-18-20_20.00sec_-15.00C_LIGHT_0301.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.UognoZAPXd (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits' -> 'wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS-calibrated image found: wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
Checking if the catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat corresponding to the image wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits
WCS catalog name: wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=7114, passed=88410
Got 88410 stars (including 81149 good ones) from the SExtractor catalog wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat
util/solve_plate_with_UCAC5 got 88410 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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits -region wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q1b1x1_2025-12-23_00-19-57_20.00sec_-14.90C_LIGHT_0303.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.FwYGdd276Q (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6382, passed=80537
Got 80537 stars (including 74028 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 80537 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 947 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits -region wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.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.odz1yGDbzr (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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=6447, passed=81526
Got 81526 stars (including 74958 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 81526 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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-54-53_20.00sec_-15.00C_LIGHT_0118.fits
Saving fully-calibrated image wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.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_2026-02-21_CI_Ori-05-Q1b1x1_215621_TTUQ1b1x1_13346_457Jz9Jw/wcs_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119.fits
Preparing the HTML report for the field Ori-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out105383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out105489.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out105615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61557.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 5s
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Considering the candidate 105380_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105380_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:55:52.85 -03:12:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105383_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105383_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:08:24.43 +00:47:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.308 3227915145558710912 077.10115314062 +00.78977416094 14.3930 13.8794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105388_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105388_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:26:23.19 +00:59:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105392_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105392_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:04:38.79 +01:13:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.344 3228750499517800320 076.16100554785 +01.22360475238 14.0238 13.5001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105393_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105393_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:27:47.45 +02:04:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105398_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105398_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:22:18.22 +00:50:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105400_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105400_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:54:56.22 -03:06:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105401_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105401_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:26:03.49 -05:20:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105403_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105403_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:19:21.78 -06:08:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 5.870 3208431077958490880 079.83914733774 -06.14343228416 14.3067 13.5788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105406_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105406_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:44:33.48 -04:56:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105408_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105408_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:41:26.71 -04:35:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105409_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105409_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:38:30.78 -01:30:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105411_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105411_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:36:23.25 -03:32:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105413_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105413_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:27:05.08 -01:43:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105417_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105417_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:05:35.78 -02:38:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.710 3214749593327072768 076.39860945118 -02.63740439787 13.5916 13.0869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105418_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105418_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:59:46.37 +01:53:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.207 3231958255972417280 074.94259496261 +01.88673225926 13.3190 12.8006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105421_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105421_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:00:13.08 -04:27:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.335 3212462982802156416 075.05389250431 -04.46551771252 13.4009 12.9162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105424_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105424_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:32:34.40 +02:45:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105426_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105426_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:51:49.66 +00:01:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105431_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105431_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:46:44.47 -00:41:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105489_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105489_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:35:45.19 -05:32:14.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
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Considering the candidate 105521_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105521_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105527_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105527_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 105536_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105536_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:56:44.20 +00:55:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105546_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105546_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105547_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105547_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 105554_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105554_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105564_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105564_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105575_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105575_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105587_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105587_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105597_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105597_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 105598_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105598_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 105600_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105600_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:25:20.97 -06:43:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.183 3208888161262384384 081.33651019102 -06.72559876286 13.6814 13.1302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105615_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 105615_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 105639_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105639_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105640_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105640_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:43:36.37 -04:11:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105641_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105641_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:49:37.80 -06:51:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105648_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105648_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105650_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105650_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 105677_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105677_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 105683_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105683_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105702_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105702_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:50:30.65 -02:56:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105712_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 105712_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 105714_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105714_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 105715_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105715_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 105717_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105717_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105731_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105731_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:27:53.48 +01:07:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.211 3221981046943590528 081.97196395401 +01.12400601939 13.9452 13.2448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105740_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105740_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 105748_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105748_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 105750_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105750_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:34:19.66 -05:30:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105751_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105751_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:25:25.84 -03:39:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105759_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105759_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105762_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105762_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 105767_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105767_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 105768_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105768_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:43:14.69 -00:23:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105769_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105769_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 105772_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105772_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:39:38.45 -06:07:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 5.493 3017068707007533696 084.90873782920 -06.11731365953 14.3459 13.3562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105775_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105775_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 105778_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105778_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 105781_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105781_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:43:09.43 -03:57:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105787_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105787_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:24:14.09 -05:57:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105791_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105791_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 105801_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105801_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 105802_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105802_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 105803_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105803_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:39:17.80 -00:56:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.435 3217527303296489472 084.82346370470 -00.94418790181 14.3605 13.4970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105807_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105807_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:55:19.90 -04:14:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.181 3212614101227705728 073.83231215771 -04.24591298690 14.1993 13.6746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105814_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105814_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:19:05.71 -05:17:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 3.757 3210038941917073664 079.77278924792 -05.29139020473 14.2611 13.3693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105815_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 105815_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 105832_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105832_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:29:29.37 -02:07:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105838_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105838_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:26:58.43 -04:16:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105847_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105847_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 105861_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 105861_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 105864_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105864_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:24:46.50 +02:58:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105967_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 105967_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 61557_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 61557_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 63280_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 63280_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:29:35.98 -06:29:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75547_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 75547_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:29:00.57 -04:41:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42977_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 42977_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:37:59.20 -01:05:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27716_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 27716_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 05:16:35.95 +00:25:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85178_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 85178_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 04:55:02.00 -03:48:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61248_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119
The candidate 61248_fd_Ori-05-Q1b1x1_2026-02-21_21-55-29_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks