This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0
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 27.4565 2461126.9565 11.77 19:49:10.30 +03:39:21.4
42.91817 -11.08744 galactic Aql Second-epoch detections are separated by 1.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.2865+03.6519 | 19:49:10.77 +03:39:23.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.2865+03.6519,2461126.9565,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.2865+03.6519 20260327.4565 11.77CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:10.30 +03:39:21.4 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295083745490644864,2461126.9565,11.82,0.05,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 4295083745490644864 20260327.4565 11.82CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:53.65 +07:14:37.4 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 14.05 19:45:39.33 +03:56:49.7
42.75241 -10.17773 galactic Aql Second-epoch detections are separated by 1.0" and 8.8 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 | ATO J296.4227+03.9511 | 19:45:39.33 +03:56:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.4227+03.9511,2461126.9565,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.4227+03.9511 20260327.4565 14.05CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:39.33 +03:56:49.7 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295905797928505984,2461126.9565,13.69,0.05,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 4295905797928505984 20260327.4565 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:57.12 +07:43:26.5 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_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
NSV 12063,2461126.9565,13.31,0.05,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
NSV 12063 20260327.4565 13.31CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:28.44 +06:33:36.3 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 13.16 19:22:41.06 +08:30:35.2
44.07473 -2.98970 galactic Aql Second-epoch detections are separated by 3.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J290.6644+08.5160 | 19:22:41.06 +08:30:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J290.6644+08.5160,2461126.9565,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.6644+08.5160 20260327.4565 13.16CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:41.06 +08:30:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4240789895640041728,2461126.9565,13.43,0.05,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 4240789895640041728 20260327.4565 13.43CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:22.97 +01:55:25.7 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 13.29 19:29:18.63 +03:00:11.5
39.96563 -7.02553 galactic Aql Second-epoch detections are separated by 0.2" and 8.8 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 | ATO J292.3314+03.0019 | 19:29:18.63 +03:00:11.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.3314+03.0019,2461126.9565,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.3314+03.0019 20260327.4565 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:18.63 +03:00:11.5 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4288966165868502272,2461126.9565,13.15,0.05,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 4288966165868502272 20260327.4565 13.15CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:21:34.67 +02:42:22.5 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_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
ASAS J192336+0755.5,2461126.9565,12.79,0.05,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 J192336+0755.5 20260327.4565 12.79CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:37.49 +07:55:15.8 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_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
ASASSN-V J194458.63+090308.4,2461126.9565,13.29,0.05,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 J194458.63+090308.4 20260327.4565 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:57.99 +09:03:00.5 ;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_Aql-02-Q2b1x1_2026-02-27_05-59-01_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 12.80 19:38:11.60 +08:58:58.6
46.31954 -6.13663 galactic Aql Second-epoch detections are separated by 3.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.5408+08.9829 | 19:38:09.65 +08:58:26.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.5408+08.9829,2461126.9565,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.5408+08.9829 20260327.4565 12.80CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:11.60 +08:58:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 12.82 19:31:55.01 +04:56:57.9
42.00405 -6.68740 galactic Aql Second-epoch detections are separated by 1.5" and 8.7 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 | ASASSN-V J193151.93+045705.9 | 19:31:51.92 +04:57:05.9 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193151.93+045705.9,2461126.9565,12.82,0.05,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 J193151.93+045705.9 20260327.4565 12.82CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:55.01 +04:56:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_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: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461126.95681932 27.03.2026 10:57:39.189 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17575
Objects passed selection criteria: 17566
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 16709.5
Average stars matched: 15994.5 (95.721 %)
Memory usage VmPeak: 122368 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 Sat Mar 28 20:44:31 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: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461126.95681932 27.03.2026 10:57:39.189 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 121
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 99 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): 182131
Objects passed selection criteria: 181747
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 157116
Average stars matched: 151230 (96.2542 %)
Memory usage VmPeak: 2010184 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 Sat Mar 28 20:48:19 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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: 2461126.95623183
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits'
wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:50.827 +06:00:03.35
Angular distance between the image centers 0.00 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 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:48.450 +05:59:26.12
Angular distance between the image centers 0.02 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 19:42:50.827 +06:00:03.35
Second-epoch second image center 19:42:48.450 +05:59:26.12
Angular distance between the image centers 0.01428 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.23SXGB7CRw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.fcUCKmqr8d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits &> /tmp/tmp.ECcG4xLOmb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits &> /tmp/tmp.UkHwumrNo6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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 12562 out of 19279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779826
a=0.000000 b=1.000000 c=22.779826
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 85 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
3.5 pix fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
2.8 pix fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Limiting magnitude estimates:
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
14.4 mag. fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
14.6 mag. fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.23SXGB7CRw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1674, passed=19279
Got 19279 stars (including 17574 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 19279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 964 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.fcUCKmqr8d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1629, passed=19357
Got 19357 stars (including 17702 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 19357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 965 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.ECcG4xLOmb (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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=940, passed=18530
Got 18530 stars (including 17585 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat
util/solve_plate_with_UCAC5 got 18530 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 967 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 967 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 - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.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.UkHwumrNo6 (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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1209, passed=20082
Got 20082 stars (including 18864 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat
util/solve_plate_with_UCAC5 got 20082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 968 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits'
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21343.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 21230_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21230_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:57:49.03 +05:57:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.091 4296621408170980096 299.45458083158 +05.95143237295 11.2884 10.4182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21231_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21231_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:19:56.71 +06:19:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21280_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21280_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:57:29.16 +08:42:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21281_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21281_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:31.56 +03:37:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21290_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21290_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:43.11 +09:55:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21292_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21292_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:05.65 +04:07:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21300_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21300_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:45:01.73 +06:09:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21301_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21301_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:56:53.16 +07:54:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21305_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21305_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:29:22.39 +07:06:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21307_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21307_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:42:55.73 +04:46:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21309_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21309_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:46:03.90 +06:55:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21311_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21311_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:51:29.66 +05:14:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21313_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21313_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:43:20.09 +04:05:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.185 4290145357712472448 295.83325538164 +04.09448873120 11.6217 10.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21316_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21316_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:37:30.53 +03:58:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21317_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21317_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:50:30.42 +08:04:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.550 4298416777528804992 297.62718099941 +08.07955349756 11.6661 11.1541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21319_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21319_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:40.61 +01:52:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21322_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21322_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:00:25.40 +02:22:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.215 4240925307368972416 300.10558297746 +02.37710442598 11.5272 10.8123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21324_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21324_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:02.06 +05:35:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21325_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 21325_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 21328_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21328_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:17.04 +03:51:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21329_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21329_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:39:37.59 +04:16:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21330_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21330_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:44:19.82 +05:09:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21332_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21332_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:50.53 +05:01:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21333_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21333_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:37.51 +05:55:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21334_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21334_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:42:19.34 +08:38:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21335_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21335_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:46:06.71 +05:41:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21337_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21337_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:37.18 +05:05:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21338_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21338_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:38:12.97 +05:50:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21342_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21342_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:49:08.88 +06:12:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21343_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 21343_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 21345_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21345_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:57.41 +04:38:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21346_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21346_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:54.54 +04:50:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21347_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21347_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:50.88 +05:31:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21348_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21348_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:49:20.16 +03:56:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.313 4242236887307122560 297.33392595566 +03.94833720544 11.3073 10.3936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21350_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21350_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:42:43.70 +02:40:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21351_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21351_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:58.42 +07:22:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21352_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21352_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:37:38.89 +06:24:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.005 4291780743832371200 294.41242189113 +06.40492412654 11.6098 10.9061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21353_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21353_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:37:30.07 +06:14:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21354_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21354_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:45:21.59 +05:37:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21355_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21355_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:27:36.16 +07:27:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21356_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21356_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:30:23.75 +03:39:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21357_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21357_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:50:29.95 +08:59:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21358_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21358_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:27.91 +05:08:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21361_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21361_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:54:28.80 +06:59:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21362_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21362_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:26.09 +04:00:49.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21363_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21363_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:07.62 +03:49:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21367_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21367_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:30:46.82 +04:58:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21368_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21368_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:43:04.57 +05:40:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21369_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21369_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:36:04.27 +06:29:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21370_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21370_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:46:24.86 +06:45:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21371_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21371_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:16.49 +04:47:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21373_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21373_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:36:41.30 +06:40:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.422 4294811272760157440 294.17242985329 +06.68011155050 11.6637 11.1062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21375_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21375_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:36:39.94 +05:10:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21379_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21379_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:26:17.66 +04:17:47.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21380_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21380_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:38:15.81 +05:55:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21381_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21381_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:59.11 +03:48:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21382_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21382_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:31:25.18 +04:21:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21383_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21383_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:38:37.00 +03:41:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.337 4290068976011924480 294.65422256718 +03.69957731875 11.5156 10.7761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21385_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21385_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:39:20.15 +06:37:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21386_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21386_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:45:22.31 +09:52:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21387_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21387_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:39:13.40 +06:16:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21388_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21388_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:35:26.63 +06:21:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21389_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21389_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:46:38.60 +05:38:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21392_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21392_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:41.48 +04:11:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.993 4290889142975460992 293.67231158447 +04.19839394801 11.8019 11.2146 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 21394_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21394_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:46.16 +04:11:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.880 4290158998529331584 295.44224408065 +04.18582801049 11.6897 11.1936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21395_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21395_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:43:11.32 +05:35:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21396_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21396_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:28:23.01 +05:19:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21397_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21397_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:51:13.49 +06:25:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21400_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21400_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:39:18.56 +06:23:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.345 4291865578019246080 294.82739388450 +06.39817532752 11.6015 10.9017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21401_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21401_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:11.85 +04:41:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21403_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21403_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:44:47.01 +08:25:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.963 4301137965729553664 296.19541780950 +08.42127872651 11.6628 11.1745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21405_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21405_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:34.32 +07:21:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21410_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21410_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:45:40.33 +06:48:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.596 4297664264898926080 296.41820991364 +06.81422808882 11.6783 11.1428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21418_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21418_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:50:47.79 +08:08:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.588 4298417464723583744 297.69917530617 +08.13345547378 11.3838 10.5167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21421_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21421_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:33.60 +05:55:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21422_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21422_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:30:01.40 +03:44:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21423_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21423_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:16.25 +06:22:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.506 4291815378439221888 295.06772561458 +06.36961053656 11.5460 10.7840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21424_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21424_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:13.25 +06:25:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21428_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21428_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:43:39.02 +07:10:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.773 4297924024521383168 295.91281829900 +07.17134385854 11.7830 11.4553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21430_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21430_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:41:37.64 +08:27:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21441_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21441_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:24:07.35 +04:19:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21446_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21446_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:22.54 +08:28:20.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21449_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21449_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:27:50.24 +07:33:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.686 4295571104013206400 291.95958973391 +07.55382872396 11.7627 11.1547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21450_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21450_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:17.26 +06:23:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21451_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 21451_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:36:28.89 +06:32:32.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Aql-02-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 ####
19:49:10.30 +03:39:21.4
19:33:53.65 +07:14:37.4
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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:50.827 +06:00:03.35
Angular distance between the image centers 0.00 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 19:42:51.800 +06:00:06.78
Second-epoch image center 19:42:48.450 +05:59:26.12
Angular distance between the image centers 0.02 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 19:42:50.827 +06:00:03.35
Second-epoch second image center 19:42:48.450 +05:59:26.12
Angular distance between the image centers 0.01428 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.xxwwRmvSau
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.on70yKRNxi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits &> /tmp/tmp.vVaevILWOL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits &> /tmp/tmp.CCdqvJlWs3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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 14938 out of 215901 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.584750
a=0.000000 b=1.000000 c=22.584750
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
3.7 pix fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
2.8 pix fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Limiting magnitude estimates:
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
14.4 mag. fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
14.6 mag. fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xxwwRmvSau (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=26960, passed=215867
Got 215867 stars (including 188619 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 215867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.on70yKRNxi (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=27226, passed=216980
Got 216980 stars (including 189460 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 216980 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 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: 0.59"
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 972 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: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.vVaevILWOL (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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=14913, passed=111072
Got 111072 stars (including 96078 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat
util/solve_plate_with_UCAC5 got 111072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 970 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.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.CCdqvJlWs3 (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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=19666, passed=147426
Got 147426 stars (including 127638 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat
util/solve_plate_with_UCAC5 got 147426 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 974 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 971 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.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_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out107849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out193227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82643.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 246992_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 246992_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 246997_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 246997_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:52:13.64 +10:03:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 5.805 4303221157996109568 298.05597111759 +10.05396231059 13.7219 13.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247004_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247004_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:53:21.50 +06:11:35.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 247013_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247013_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:14.16 +03:47:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.015 4289380200711184768 293.05940816541 +03.79049026759 13.5024 12.9004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247015_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247015_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247029_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247029_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:21:50.43 +09:43:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 247038_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247038_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:56:53.72 +09:40:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247040_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247040_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:29:46.31 +07:20:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 247057_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247057_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:54:11.91 +01:52:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.569 4240625106335236352 298.55029709588 +01.88186988718 13.3733 12.9227 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 247062_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247062_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:17:18.46 +09:29:43.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 247066_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247066_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:48:49.14 +02:03:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.310 4241428230859691392 297.20478004170 +02.06316923291 13.2761 12.7477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247067_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247067_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:03:58.85 +08:26:30.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 247071_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247071_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247074_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247074_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:21:35.23 +09:49:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.466 4308651272290571008 290.39683576903 +09.83048959342 11.4740 9.9231 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247095_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247095_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 247096_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247096_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:58:18.38 +08:26:29.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 247099_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247099_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:00:12.12 +09:46:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.410 4300075734409539712 300.05010255324 +09.77344438979 12.6215 11.4582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247100_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247100_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247109_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247109_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247111_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247111_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247122_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247122_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:33:16.95 +03:50:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 247133_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247133_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247140_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247140_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 247153_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247153_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:34:38.75 +08:24:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.779 4296061997264464512 293.66195936950 +08.41531408253 12.7966 11.8289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247162_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247162_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:29:50.36 +09:52:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.485 4314468788326096000 292.46040705689 +09.87283516689 11.1591 9.7538 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247165_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247165_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:27:34.83 +04:48:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.970 4292692994889449984 291.89497666089 +04.79977484324 12.8696 12.0397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247166_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 247166_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 247167_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247167_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 247168_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247168_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:23:04.58 +07:54:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.818 4295830485711558144 290.76959251215 +07.91074836543 12.6910 11.8157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247179_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247179_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:56:10.13 +08:04:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.917 4298275829571776896 299.04231535069 +08.07759286639 10.9632 9.6492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247732_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247732_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:48:25.45 +04:09:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247854_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247854_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:06:22.43 +08:28:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247869_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247869_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:22:49.91 +02:09:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247902_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247902_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:57:18.56 +03:34:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247911_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247911_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:58:31.63 +05:44:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.041 4248563408490536704 299.63109665974 +05.73468172204 14.1777 13.7172 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247912_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247912_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:59:26.57 +05:22:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247939_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247939_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:04:39.88 +06:04:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247943_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247943_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:58:47.77 +10:06:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.622 4300287218599347200 299.69891945961 +10.10851021868 14.1692 13.6852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247949_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247949_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:00:07.40 +08:45:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247950_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247950_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:00:56.35 +05:28:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.939 4248866427021364736 300.23492342111 +05.46867195966 14.4243 13.9171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247952_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247952_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:03:58.72 +06:38:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247955_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247955_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:56:20.32 +09:11:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.870 4299915033914157952 299.08363888132 +09.19903378862 14.1147 13.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247957_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247957_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:57:54.32 +08:41:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247962_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247962_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:53:44.34 +06:34:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247965_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247965_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:52:11.88 +06:17:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.362 4296876945848669440 298.04940372803 +06.28482839110 14.1753 13.6212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247967_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 247967_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 20:05:29.62 +07:27:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174553_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 174553_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:43.13 +09:55:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44257_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 44257_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:40:42.83 +03:12:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228034_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 228034_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:32:24.71 +08:10:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.477 4296036815912028032 293.10208149419 +08.17013949552 11.2597 9.8077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70827_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 70827_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:51:29.56 +04:27:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227822_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 227822_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 32889_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 32889_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:28:31.21 +02:36:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27048_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 27048_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:16:16.00 +02:15:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165804_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 165804_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:57:29.18 +08:42:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193227_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 193227_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 105185_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 105185_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:23:07.74 +05:55:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82643_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
Preparing report for the candidate 82643_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
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Considering the candidate 125952_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 125952_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:46:03.90 +06:55:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196611_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 196611_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:17:07.81 +08:41:17.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)
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Considering the candidate 60712_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 60712_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:17:29.44 +03:53:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96747_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 96747_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks
**** FOUND 19:54:33.57 +05:41:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107849_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518
The candidate 107849_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518 did not pass the final checks