This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 29.3550 2461128.8550 12.85 18:17:46.63 -12:43:31.4
17.78888 1.52442 galactic Ser Second-epoch detections are separated by 4.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4153498190053529088 | 18:17:46.16 -12:43:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 17 46.63 -12 43 31.4 12.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4153498190053529088,2461128.8550,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4153498190053529088 20260329.3550 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:17:46.63 -12:43:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 19 59.94 -06 17 52.4 13.1 U Ser 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
ZTF J182000.04-061800.9,2461128.8550,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J182000.04-061800.9 20260329.3550 13.09CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:19:59.94 -06:17:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 08 10.77 -12 25 33.5 12.2 U Ser 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,2461128.8550,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.3550 12.22CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:10.77 -12:25:33.5 ;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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 07 55.48 -08 39 50.8 12.8 U Ser 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
ASASSN-V J180755.71-083947.8,2461128.8550,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180755.71-083947.8 20260329.3550 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:55.48 -08:39:50.8 ;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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1756504-062553,2461128.8550,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1756504-062553 20260329.3550 12.49CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:56:50.50 -06:25:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 05 52.16 -06 53 19.7 13.1 U Ser 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
ZTF J180552.18-065319.5,2461128.8550,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J180552.18-065319.5 20260329.3550 13.08CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:52.16 -06:53:19.7 ;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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 09 30.52 -06 51 16.8 12.9 U Ser 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
NSVS J1809306-065115,2461128.8550,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1809306-065115 20260329.3550 12.89CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:30.52 -06:51:16.8 ;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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 08 53.05 -07 18 06.5 12.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4171067316398094208,2461128.8550,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4171067316398094208 20260329.3550 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:53.05 -07:18:06.5 ;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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 05 47.53 -13 11 19.3 11.2 U Ser 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
ASAS J180548-1311.3,2461128.8550,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180548-1311.3 20260329.3550 11.19CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:47.53 -13:11:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3550* 18 02 05.40 -13 49 58.1 12.7 U Ser 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
ASASSN-V J180205.45-135000.5,2461128.8550,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180205.45-135000.5 20260329.3550 12.68CV 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:02:05.40 -13:49:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20_00sec_-15_00C_LIGHT_0313_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: 2461099.01462919 27.02.2026 12:20:53.962 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
First image: 2461099.01462919 27.02.2026 12:20:53.962 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Last image: 2461128.85533891 29.03.2026 08:31:31.282 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5152
Objects passed selection criteria: 5141
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 4454.25
Average stars matched: 4376 (98.2433 %)
Memory usage VmPeak: 112300 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:33:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.01462919 27.02.2026 12:20:53.962 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
First image: 2461099.01462919 27.02.2026 12:20:53.962 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Last image: 2461128.85533891 29.03.2026 08:31:31.282 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 130
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.02
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: 15 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): 55296
Objects passed selection criteria: 55209
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 46189.2
Average stars matched: 44328.5 (95.9715 %)
Memory usage VmPeak: 161524 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:34:35 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
SExtractor catalog cache: saved Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat to cache
SExtractor catalog cache: saved Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.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: 2461128.85475170
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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits'
wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits exists and is non-empty
Saving wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits to local_wcs_cache/
'wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits' -> 'local_wcs_cache/wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits'
wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits exists and is non-empty
Saving wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits to local_wcs_cache/
'wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits' -> 'local_wcs_cache/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits'
wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits exists and is non-empty
Saving wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits to local_wcs_cache/
'wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits' -> 'local_wcs_cache/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:00.484 -09:59:36.93
Second-epoch image center 18:00:16.943 -10:02:14.77
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 18:00:00.484 -09:59:36.93
Second-epoch image center 18:00:14.400 -10:01:51.43
Angular distance between the image centers 0.07 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 18:00:16.943 -10:02:14.77
Second-epoch second image center 18:00:14.400 -10:01:51.43
Angular distance between the image centers 0.01228 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits &> /tmp/tmp.ObnbTPUTbn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits &> /tmp/tmp.HognJhdstm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits &> /tmp/tmp.WWfxIkX3LE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits &> /tmp/tmp.t7uecQ3ZxF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
Found non-empty wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
The reference image (wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits) and catalog (wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat) found
'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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 4799 out of 8050 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.923277
a=0.000000 b=1.000000 c=22.923277
From vast_summary.log: estimated ref. image limiting mag.: -8.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.54
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
2.5 pix Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
3.1 pix fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
3.1 pix fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Limiting magnitude estimates:
14.5 mag. Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
14.5 mag. Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
13.7 mag. fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
13.7 mag. fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ObnbTPUTbn (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_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits' -> 'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Checking if the catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS catalog name: wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=623, passed=8050
Got 8050 stars (including 7407 good ones) from the SExtractor catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 8050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 923 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits -region wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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.HognJhdstm (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_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits' -> 'wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS-calibrated image found: wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Checking if the catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS catalog name: wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=7634
Got 7634 stars (including 7012 good ones) from the SExtractor catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat
util/solve_plate_with_UCAC5 got 7634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits -region wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.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.WWfxIkX3LE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Checking if the catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS catalog name: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=277, passed=4228
Got 4228 stars (including 3949 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat
util/solve_plate_with_UCAC5 got 4228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 916 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 913 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits -region wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.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.t7uecQ3ZxF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Checking if the catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS catalog name: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=257, passed=4259
Got 4259 stars (including 3999 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 4259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 917 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
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 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.75"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits -region wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits'
Saving fully-calibrated image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits'
Saving fully-calibrated image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits'
Preparing the HTML report for the field Oph-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20290_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 20290_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:59:00.79 -11:33:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20300_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 20300_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:54:33.88 -10:14:33.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Oph-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
SExtractor catalog cache: saved Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat to cache
SExtractor catalog cache: saved Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits exists and is non-empty
wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits exists and is non-empty
wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits exists and is non-empty
wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:00:00.484 -09:59:36.93
Second-epoch image center 18:00:16.943 -10:02:14.77
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 18:00:00.484 -09:59:36.93
Second-epoch image center 18:00:14.400 -10:01:51.43
Angular distance between the image centers 0.07 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 18:00:16.943 -10:02:14.77
Second-epoch second image center 18:00:14.400 -10:01:51.43
Angular distance between the image centers 0.01228 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/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits &> /tmp/tmp.y5LbAr4toK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits &> /tmp/tmp.anV6EZlfmK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits &> /tmp/tmp.ZWWEad9qKV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits &> /tmp/tmp.6lqsy1VhdZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
Found non-empty wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits and wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
The reference image (wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits) and catalog (wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat) found
'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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 5581 out of 76417 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.677520
a=0.000000 b=1.000000 c=22.677520
From vast_summary.log: estimated ref. image limiting mag.: -8.02
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.66
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
2.2 pix Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
2.6 pix fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
2.7 pix fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Limiting magnitude estimates:
14.7 mag. Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
14.6 mag. Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
14.0 mag. fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
14.0 mag. fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.y5LbAr4toK (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_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits' -> 'wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Checking if the catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
WCS catalog name: wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=5482, passed=76410
Got 76410 stars (including 70820 good ones) from the SExtractor catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 76410 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits -region wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.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.anV6EZlfmK (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_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits' -> 'wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS-calibrated image found: wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Checking if the catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat corresponding to the image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
WCS catalog name: wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4994, passed=75317
Got 75317 stars (including 70185 good ones) from the SExtractor catalog wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat
util/solve_plate_with_UCAC5 got 75317 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits -region wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.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.ZWWEad9qKV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Checking if the catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
WCS catalog name: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1799, passed=36286
Got 36286 stars (including 34454 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat
util/solve_plate_with_UCAC5 got 36286 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 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 920 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits -region wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.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.6lqsy1VhdZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS-calibrated image found: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Checking if the catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
WCS catalog name: wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1726, passed=36047
Got 36047 stars (including 34281 good ones) from the SExtractor catalog wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 36047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 922 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits -region wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.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_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits
Saving fully-calibrated image wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits
Saving fully-calibrated image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-30-40_20.00sec_-15.00C_LIGHT_0313.fits
Saving fully-calibrated image wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Oph-06-Q2b1x1_033217_TTUQ2b1x1_16457_WDo44kII/wcs_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314.fits
Preparing the HTML report for the field Oph-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out87071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out92141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out92999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out18159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93196.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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 92999_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 92999_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:21:17.06 -10:43:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.569 4154351715996408960 275.32065425391 -10.72421459685 12.9138 12.1132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93008_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 93008_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 93010_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 93010_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 93011_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93011_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:37:38.05 -12:10:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93012_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93012_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:52:06.19 -05:44:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93014_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93014_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:08:41.02 -13:29:23.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 93016_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93016_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:38:13.54 -13:28:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.414 4161447899658435200 264.55681937404 -13.47936351089 13.0255 12.1878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93019_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93019_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:32:53.10 -06:14:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93028_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93028_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:24:51.53 -11:19:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93090_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93090_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:39:59.90 -09:32:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 1.396 4165068694497031552 264.99924229715 -09.53319563033 10.8867 9.6538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93160_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93160_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:34:42.85 -11:13:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 93166_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93166_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:24:51.27 -11:01:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93196_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 93196_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 93229_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93229_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:47:37.73 -08:24:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93234_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93234_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:44:28.93 -08:04:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.373 4168679658176411264 266.12092404936 -08.06968452518 12.3712 11.2772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93252_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93252_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:33:00.55 -07:42:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93255_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93255_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:59:36.59 -09:28:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93278_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93278_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:51:34.52 -06:50:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.091 4171872777382400256 267.89425538153 -06.84443006225 12.5513 11.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93296_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93296_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:33:57.24 -13:28:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.629 4161632991237942400 263.48943461964 -13.48138195451 12.6237 11.5442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93298_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93298_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:43:42.39 -10:44:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93306_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93306_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:34:57.93 -07:14:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.961 4169381872450232960 263.74189582313 -07.24731137858 12.8455 11.8909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93319_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93319_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:56:12.48 -07:23:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.458 4171672498778009600 269.05207038223 -07.38532855491 13.1548 12.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93339_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93339_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:46:28.59 -08:34:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 3.416 4165565566372706816 266.61817227820 -08.57397050912 12.7383 11.6324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93340_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93340_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:38:54.34 -10:11:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93345_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93345_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:44:53.09 -13:16:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93368_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93368_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:44:26.73 -13:03:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.030 4149889313695335808 266.11029861979 -13.05477476060 12.7427 11.8206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93388_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93388_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:20:16.26 -06:26:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93399_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93399_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:41:40.09 -10:23:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93406_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93406_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:38:14.64 -09:54:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93413_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93413_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:59:26.11 -06:08:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.659 4172159857304322688 269.85939787264 -06.13517685014 13.0589 12.0218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93417_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93417_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:05:48.75 -06:13:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93419_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93419_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:32:41.84 -08:51:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93424_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93424_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:51:36.92 -11:59:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93426_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93426_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:39:43.66 -06:01:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93428_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93428_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:07:20.03 -07:55:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93446_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93446_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:42:19.51 -12:05:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93452_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93452_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:11:44.38 -05:59:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.310 4172818804061182080 272.93529659674 -05.98964172688 11.6254 10.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93454_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93454_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:08:29.49 -08:49:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93458_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93458_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:47:52.77 -12:12:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93463_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93463_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:55:50.23 -12:47:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.309 4151231718645917056 268.95930805320 -12.79669357825 14.0324 11.7675 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93466_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93466_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:57:01.21 -06:54:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93470_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93470_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:43:33.88 -05:52:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93478_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93478_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:41:55.68 -07:52:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.165 4168721959318352768 265.48216521175 -07.87799546348 13.9038 13.1374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93481_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93481_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:01:44.45 -10:40:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93482_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93482_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:54:23.62 -06:59:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93486_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93486_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:32:06.58 -13:45:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93490_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93490_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:54:07.76 -08:39:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93491_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93491_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:10:48.96 -07:12:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.315 4171083499834485376 272.70502481448 -07.20828175719 13.0013 11.6471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93494_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93494_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:36:58.31 -10:26:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93496_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93496_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:39:19.87 -06:41:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.021 4169809578173463040 264.83347943111 -06.68693170277 11.5888 9.9125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 93504_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93504_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:33:59.89 -06:11:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.933 4170077652852184064 263.49906713218 -06.18566020067 12.9342 11.5498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93508_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93508_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:44:11.40 -06:40:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.041 4169108295913565312 266.04748246546 -06.67176077065 13.6019 12.7521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93511_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93511_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:33:04.73 -10:36:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93532_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93532_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:45:38.85 -09:26:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.563 4164955371779873664 266.41219981040 -09.43551519519 12.1727 10.6777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93541_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93541_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:47:38.21 -07:33:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.843 4165792993478447104 266.90931879627 -07.55645704497 13.7449 12.7990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93544_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93544_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:43:23.05 -06:00:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.281 4175211036425929984 265.84608024187 -06.01622965007 13.4460 12.3253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93549_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93549_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:50:51.49 -07:02:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.212 4171828560708399744 267.71420870442 -07.04293572014 12.9987 11.7418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93557_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93557_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:47:16.13 -09:19:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93567_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93567_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:45:28.43 -08:38:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93574_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93574_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:51:20.17 -06:44:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.131 4171877592055324416 267.83419144596 -06.74655454337 12.8495 11.4395 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93577_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 93577_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:48:42.16 -07:06:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.518 4174838130188096512 267.17589022023 -07.10874743760 13.5793 12.6181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71693_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 71693_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:06:42.65 -08:13:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73514_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 73514_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87971_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 87971_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:04:54.73 -13:02:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.993 4150648079803582080 271.22859603863 -13.03592761231 11.3574 9.7831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73507_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 73507_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 87071_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 87071_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:07:04.76 -11:30:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.311 4151094451481455232 271.76957598059 -11.51370702343 10.5595 8.9874 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 86547_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 86547_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 18:14:03.75 -06:14:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74764_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 74764_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 75216_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 75216_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 65924_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 65924_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:52:31.68 -08:54:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74191_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 74191_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 33403_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 33403_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:58:01.42 -12:25:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25240_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 25240_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 92141_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 92141_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:51:56.21 -13:52:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.744 4148893229232423040 267.98463705015 -13.88241451629 13.2069 10.9924 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 41190_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 41190_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:59:00.79 -11:33:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19296_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 19296_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks
**** FOUND 17:54:52.56 -13:43:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18159_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
Preparing report for the candidate 18159_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
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Considering the candidate 17352_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314
The candidate 17352_fd_Oph-06-Q2b1x1_2026-03-29_03-31-31_20.00sec_-15.00C_LIGHT_0314 did not pass the final checks