This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F
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 27.3980 2461126.8980 12.77 20:07:26.83 +07:54:36.8
48.98844 -12.96027 galactic Aql Second-epoch detections are separated by 3.5" and 2.0 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 | Gaia DR3 4250796615381681408 | 20:07:27.36 +07:54:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4250796615381681408,2461126.8980,12.77,0.05,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
Gaia DR3 4250796615381681408 20260327.3980 12.77CV 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:26.83 +07:54:36.8 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3980 2461126.8980 12.73 19:54:38.86 +07:13:37.8
46.77088 -10.54878 galactic Aql Second-epoch detections are separated by 5.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.6562+07.2375 | 19:54:39.37 +07:13:39.7 (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 J298.6562+07.2375,2461126.8980,12.73,0.05,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 J298.6562+07.2375 20260327.3980 12.73CV 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:38.86 +07:13:37.8 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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
target,2461126.8980,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3980 12.60CV 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:35.27 +08:15:03.9 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3980 2461126.8980 12.62 19:22:50.14 +08:25:15.2
44.01373 -3.06447 galactic Aql Second-epoch detections are separated by 4.8" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J290.6935+08.4184 | 19:22:49.27 +08:25:22.7 (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 J290.6935+08.4184,2461126.8980,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.6935+08.4184 20260327.3980 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:50.14 +08:25:15.2 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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
V0422 Aql,2461126.8980,12.57,0.05,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
V0422 Aql 20260327.3980 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:18.33 +06:22:43.6 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3980 2461126.8980 12.20 19:17:01.90 +02:44:46.1
38.30710 -4.42887 galactic Aql Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4267982978552285056 | 19:17:02.20 +02:44:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4267982978552285056,2461126.8980,12.20,0.05,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 4267982978552285056 20260327.3980 12.20CV 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:17:01.90 +02:44:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3980 2461126.8980 12.32 19:18:39.11 +01:55:04.5
37.75709 -5.17005 galactic Aql Second-epoch detections are separated by 4.2" and 1.7 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 | Gaia DR3 4264878644913985792 | 19:18:39.20 +01:55:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4264878644913985792,2461126.8980,12.32,0.05,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 4264878644913985792 20260327.3980 12.32CV 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:39.11 +01:55:04.5 ;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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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_04-33-21_20_00sec_-15_00C_LIGHT_0423_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_04-32-38_20_00sec_-15_00C_LIGHT_0422_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: 2461126.89828601 27.03.2026 09:33:21.911 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
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): 15536
Objects passed selection criteria: 15492
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 12348.5
Average stars matched: 12027 (97.3964 %)
Memory usage VmPeak: 121548 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 Fri Mar 27 06:00:04 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: 2461126.89828601 27.03.2026 09:33:21.911 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 144
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: 38 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): 178614
Objects passed selection criteria: 178128
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 128282
Average stars matched: 122864 (95.7763 %)
Memory usage VmPeak: 1944648 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 Fri Mar 27 06:04:54 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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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: 2461126.89778444
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits'
wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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 19:42:49.031 +06:00:54.77
Angular distance between the image centers 0.02 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 19:42:48.797 +06:00:46.38
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 19:42:49.031 +06:00:54.77
Second-epoch second image center 19:42:48.797 +06:00:46.38
Angular distance between the image centers 0.00252 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.XZqOtiKA6v
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.NoDfIqGzkh
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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits &> /tmp/tmp.2N8DNVMFEG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits &> /tmp/tmp.CsNoZbSpQ0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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 10 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
4.0 pix fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
3.1 pix fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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
13.6 mag. fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
13.7 mag. fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.1 (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.XZqOtiKA6v (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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.NoDfIqGzkh (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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.2N8DNVMFEG (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=240, passed=8119
Got 8119 stars (including 7876 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 8119 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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: 0.76"
Estimated accuracy of the plate solution: 0.80"
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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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.CsNoZbSpQ0 (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=287, passed=9563
Got 9563 stars (including 9270 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 9563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
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: 0.75"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 969 stars left (next iteration limit 1064)
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_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits'
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21238_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 21238_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:50:59.29 +08:51:14.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07462_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 07462_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:39:11.70 +05:23:54.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07529_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 07529_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:33:46.14 +05:27:56.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10981_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 10981_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:34:05.91 +07:22:39.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09249_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 09249_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:55:18.75 +06:24:12.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13675_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 13675_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:50:47.88 +08:52:10.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13132_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 13132_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:54:15.01 +08:27:38.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01838_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 01838_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:29:01.06 +01:57:01.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10843_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 10843_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:04:08.33 +07:16:40.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03657_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 03657_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:25:30.56 +03:06:58.8 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 ####
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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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 19:42:49.031 +06:00:54.77
Angular distance between the image centers 0.02 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 19:42:48.797 +06:00:46.38
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 19:42:49.031 +06:00:54.77
Second-epoch second image center 19:42:48.797 +06:00:46.38
Angular distance between the image centers 0.00252 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.jxiC1ErTz9
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.VCIndEn7hc
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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits &> /tmp/tmp.g4ei8PV83v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits &> /tmp/tmp.UCmiRIPCr7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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 89 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
4.2 pix fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
3.2 pix fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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
13.6 mag. fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
13.8 mag. fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jxiC1ErTz9 (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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.VCIndEn7hc (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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.g4ei8PV83v (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4506, passed=53077
Got 53077 stars (including 48547 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 53077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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: 0.70"
Estimated accuracy of the plate solution: 0.74"
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_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.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.UCmiRIPCr7 (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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=5441, passed=73365
Got 73365 stars (including 67872 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 73365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 969 stars left (next iteration limit 1064)
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_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits -region wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/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_04-32-38_20.00sec_-15.00C_LIGHT_0422.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-32-38_20.00sec_-15.00C_LIGHT_0422.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.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_2026-03-27_CI_Aql-02-Q2b1x1_055739_TTUQ2b1x1_774_bT3Y3f6F/wcs_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423.fits
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out182228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out247006.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out113492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36528.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 3s
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Considering the candidate 246994_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 246994_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:54:18.95 +07:58:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.737 4298188555839495424 298.57928079312 +07.97731793478 13.3750 12.9101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246999_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 246999_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
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Considering the candidate 247000_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247000_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:57:18.12 +03:01:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.838 4241210321399246592 299.32547126659 +03.02754579091 12.1307 11.5644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247001_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247001_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:25:21.98 +03:26:55.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 247002_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 247002_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
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Considering the candidate 247004_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247004_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:02:37.34 +05:55:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.791 4248907349470536832 300.65423872050 +05.92050496257 12.8115 12.2623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247006_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247006_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:33:41.80 +09:04:16.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 247012_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247012_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:50:20.13 +03:06:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 247017_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 247017_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
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Considering the candidate 247022_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247022_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:18:50.80 +02:28:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.819 4291931480013045504 289.71147526822 +02.48109874941 12.2770 11.3433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247023_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247023_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:15:20.77 +08:22:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.384 4308057261137728640 288.83721081994 +08.37453791549 12.5450 11.9973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247027_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247027_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:22:48.74 +07:29:13.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 247040_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 247040_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
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Considering the candidate 247049_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247049_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:17:39.47 +01:56:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.446 4264868336992473728 289.41374128841 +01.94705118719 12.2713 11.0249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247050_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247050_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:30:14.33 +10:08:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.227 4314482424804814976 292.55972694679 +10.14738144529 12.6134 12.0982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 247122_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247122_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247137_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247137_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:32:58.61 +05:01:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247164_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247164_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247178_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247178_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:55:28.01 +06:24:04.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 247198_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247198_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247202_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247202_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:04:13.51 +07:15:39.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247220_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247220_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 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 247273_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247273_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247305_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247305_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247333_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247333_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 247356_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247356_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247367_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247367_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247374_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247374_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247381_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247381_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247383_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247383_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247386_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247386_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 247388_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247388_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247389_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247389_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 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 247390_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247390_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 247392_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247392_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 247396_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 247396_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 94260_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 94260_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:39:11.69 +05:23:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182228_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 182228_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:07:25.50 +09:33:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.585 4299586348656726912 301.85782249395 +09.55867926907 9.8023 8.0944 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175254_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 175254_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:47:35.98 +09:56:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70827_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 70827_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:51:29.66 +04:27:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228247_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 228247_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:05:51.53 +09:38:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44257_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 44257_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:40:42.88 +03:12:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32889_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 32889_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:28:31.31 +02:36:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27048_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 27048_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:16:16.02 +02:15:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113492_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 113492_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
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Considering the candidate 164556_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 164556_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 165804_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 165804_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:57:29.16 +08:42:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125952_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 125952_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:46:03.89 +06:55:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105185_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 105185_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:23:07.68 +05:55:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41045_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 41045_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:43:36.94 +03:02:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36528_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 36528_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20436_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
Preparing report for the candidate 20436_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174553_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 174553_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:40:43.17 +09:55:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68247_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 68247_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:45:57.46 +04:14:54.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103275_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 103275_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:31:43.44 +05:46:09.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101391_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 101391_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:47:46.14 +05:46:55.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160815_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 160815_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:42:45.83 +08:22:58.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107899_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 107899_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:36:12.69 +06:00:26.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144172_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 144172_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:45:40.06 +07:36:47.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141641_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 141641_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:32:00.74 +07:29:14.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70962_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 70962_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:53:22.59 +04:24:02.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149399_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 149399_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:50:17.45 +07:54:09.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79986_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 79986_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:27:41.15 +04:42:35.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199123_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 199123_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:44:41.38 +08:43:34.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49609_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 49609_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:38:48.98 +03:22:54.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40420_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 40420_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:35:25.15 +02:54:50.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99865_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 99865_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:33:46.13 +05:27:56.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64595_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 64595_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:51:26.82 +04:05:19.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140163_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 140163_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:34:05.92 +07:22:39.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88225_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 88225_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:33:07.86 +05:01:45.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131670_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 131670_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:54:40.23 +07:08:25.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182513_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 182513_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:44:01.81 +09:31:02.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119222_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 119222_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:55:18.74 +06:24:12.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165917_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 165917_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:50:47.87 +08:52:10.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163377_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 163377_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:54:15.00 +08:27:38.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180912_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 180912_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:51:17.76 +09:37:47.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52836_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 52836_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:30:33.16 +03:26:40.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23029_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 23029_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:31:05.16 +02:00:41.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41505_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 41505_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:30:10.67 +02:54:15.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78203_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 78203_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:03:12.54 +04:43:48.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41305_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 41305_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:28:20.87 +02:55:48.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178226_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 178226_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:18:52.85 +09:37:03.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172862_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 172862_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:22:48.40 +09:54:50.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24509_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 24509_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:17:48.08 +02:01:52.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165118_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 165118_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:00:58.94 +08:33:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47546_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 47546_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:25:30.54 +03:06:58.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21985_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 21985_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 19:29:01.05 +01:57:01.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134884_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 134884_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks
**** FOUND 20:04:08.29 +07:16:40.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83501_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423
The candidate 83501_fd_Aql-02-Q2b1x1_2026-03-27_04-33-21_20.00sec_-15.00C_LIGHT_0423 did not pass the final checks