This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4316205020251518080,2461126.8920,12.94,0.05,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 4316205020251518080 20260327.3920 12.94CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:03.50 +12:49:27.1 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1823997985615736576,2461126.8920,12.94,0.05,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 1823997985615736576 20260327.3920 12.94CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:29.59 +17:24:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4318706271792510208,2461126.8920,12.83,0.05,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 4318706271792510208 20260327.3920 12.83CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:50.84 +15:27:59.5 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3920 2461126.8920 12.73 19:57:45.90 +14:19:06.1
53.37698 -7.66200 galactic Aql Second-epoch detections are separated by 0.3" and 7.1 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 J299.4345+14.3209 | 19:57:45.90 +14:19:06.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.355+/-0.045 (G)
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 J299.4345+14.3209,2461126.8920,12.73,0.05,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 J299.4345+14.3209 20260327.3920 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:45.90 +14:19:06.1 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_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
ZTF J194025.38+164744.1,2461126.8920,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194025.38+164744.1 20260327.3920 12.71CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:25.29 +16:47:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3920 2461126.8920 12.72 19:48:49.09 +11:12:54.1
49.56569 -7.33142 galactic Aql Second-epoch detections are separated by 7.9" and 8.1 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 4303602658480015488 | 19:48:50.25 +11:13:00.7 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4303602658480015488,2461126.8920,12.72,0.05,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 4303602658480015488 20260327.3920 12.72CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:49.09 +11:12:54.1 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_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
ZTF J195411.86+173235.0,2461126.8920,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195411.86+173235.0 20260327.3920 12.70CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:12.80 +17:32:20.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4314102135588181248,2461126.8920,12.61,0.05,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 4314102135588181248 20260327.3920 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:25.24 +13:04:40.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_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
SU Sge,2461126.8920,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SU Sge 20260327.3920 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:01.17 +17:34:32.8 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190528+1720.1,2461126.8920,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190528+1720.1 20260327.3920 12.36CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:05:30.20 +17:20:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_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
Dauban V385,2461126.8920,13.06,0.05,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
Dauban V385 20260327.3920 13.06CV 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:40.72 +15:31:08.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20_00sec_-14_90C_LIGHT_0411_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: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461126.89226351 27.03.2026 09:24:41.567 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
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: 5 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): 16855
Objects passed selection criteria: 16813
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 13961.8
Average stars matched: 13567.5 (97.1762 %)
Memory usage VmPeak: 123236 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 05:43:46 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: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461126.89226351 27.03.2026 09:24:41.567 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 105
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 52 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): 183034
Objects passed selection criteria: 182587
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 136174
Average stars matched: 130564 (95.8797 %)
Memory usage VmPeak: 2017608 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 05:48:55 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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: 2461126.89170310
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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits'
wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:07.829 +14:01:31.18
Angular distance between the image centers 0.06 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 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:09.864 +14:01:00.24
Angular distance between the image centers 0.05 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 19:33:07.829 +14:01:31.18
Second-epoch second image center 19:33:09.864 +14:01:00.24
Angular distance between the image centers 0.01190 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.jBQ4ChDQc2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.q2ykmI1bQw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits &> /tmp/tmp.CcipsWd4ED
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits &> /tmp/tmp.2fxmLw5S55
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
Found non-empty wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
The reference image (wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits) and catalog (wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat) found
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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 11734 out of 22299 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846247
a=0.000000 b=1.000000 c=22.846247
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.82
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.82
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.2 pix Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
3.2 pix fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
3.4 pix fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Limiting magnitude estimates:
14.8 mag. Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
14.8 mag. Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
13.9 mag. fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
13.8 mag. fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.3 (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.jBQ4ChDQc2 (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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2194, passed=22299
Got 22299 stars (including 20069 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 22299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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: 0.65"
Estimated accuracy of the plate solution: 0.48"
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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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.q2ykmI1bQw (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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2174, passed=22325
Got 22325 stars (including 20124 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 22325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 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: 0.57"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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.CcipsWd4ED (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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, passed=11611
Got 11611 stars (including 11092 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 11611 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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: 0.66"
Estimated accuracy of the plate solution: 0.73"
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-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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.2fxmLw5S55 (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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=494, passed=11017
Got 11017 stars (including 10516 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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: 0.76"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits'
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31538_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 31538_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:40:43.02 +09:55:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06341_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 06341_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:24:59.63 +11:57:00.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05857_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 05857_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:42:33.98 +11:49:38.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18016_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 18016_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:41:03.00 +17:28:32.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20126_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 20126_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:40:05.85 +18:00:49.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03355_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 03355_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:46:15.36 +10:36:54.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03096_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 03096_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:51:02.02 +10:24:55.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10684_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 10684_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:24.71 +13:51:49.7 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-01-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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:07.829 +14:01:31.18
Angular distance between the image centers 0.06 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 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:09.864 +14:01:00.24
Angular distance between the image centers 0.05 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 19:33:07.829 +14:01:31.18
Second-epoch second image center 19:33:09.864 +14:01:00.24
Angular distance between the image centers 0.01190 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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.RX49ubksJa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.cYfu0kCuaf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits &> /tmp/tmp.rF1pqEWNFt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits &> /tmp/tmp.JuEbcqpzSf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
Found non-empty wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
The reference image (wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits) and catalog (wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat) found
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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 13769 out of 233554 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.663569
a=0.000000 b=1.000000 c=22.663569
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 79 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.0 pix Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
3.3 pix fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
3.5 pix fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Limiting magnitude estimates:
15.0 mag. Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
15.0 mag. Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
13.9 mag. fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
13.9 mag. fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.2 (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.RX49ubksJa (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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=33990, passed=233515
Got 233515 stars (including 199167 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 233515 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 978 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: 0.51"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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.cYfu0kCuaf (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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=33841, passed=234267
Got 234267 stars (including 200046 good ones) from the SExtractor catalog wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 234267 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 976 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 976 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: 0.51"
Excluding outliers - 973 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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.rF1pqEWNFt (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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=7090, passed=81550
Got 81550 stars (including 74404 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 81550 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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: 0.65"
Estimated accuracy of the plate solution: 0.71"
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_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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.JuEbcqpzSf (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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=6840, passed=74817
Got 74817 stars (including 67911 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 74817 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-23-53_20.00sec_-14.90C_LIGHT_0411.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.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-01-Q2b1x1_053939_TTUQ2b1x1_5042_z6u3fkDg/wcs_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412.fits
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out246080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out152514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out228052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265394.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 264969_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264969_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:25:15.97 +15:23:36.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 264973_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264973_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:58:13.68 +13:44:57.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 264980_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264980_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:44:49.24 +12:15:31.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 264983_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264983_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:30:21.66 +12:12:41.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 264984_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264984_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:55:02.74 +17:21:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 264985_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 264985_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 264986_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264986_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:43.73 +11:29:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264987_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264987_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:08:52.49 +14:51:20.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 264991_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 264991_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:52:04.14 +17:23:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.732 1821174199214899456 298.01860363426 +17.38821602478 12.5963 12.3342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264997_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 264997_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265000_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265000_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:14.97 +14:42:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 265001_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265001_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:53:22.52 +15:38:33.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 265002_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265002_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265003_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265003_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265004_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265004_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:36:28.85 +09:51:53.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 265005_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265005_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:41:21.88 +18:05:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265006_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265006_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:49:35.33 +16:46:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 265007_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265007_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265008_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265008_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:40:24.27 +11:45:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 265011_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265011_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:50:52.81 +16:46:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.758 1820760641076872320 297.71860972591 +16.76878744662 12.0498 10.8617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265012_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265012_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265014_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265014_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:55.89 +16:43:36.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)
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Considering the candidate 265015_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265015_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265016_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265016_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:48:59.62 +16:05:42.4 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 265017_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265017_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:08:47.01 +14:38:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.171 4320461332888586368 287.19514854282 +14.63522479839 11.4446 9.7898 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265028_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265028_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:52:37.16 +15:02:21.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)
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Considering the candidate 265361_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265361_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:51.01 +12:47:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265394_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 265394_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 265412_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265412_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:38:29.63 +17:14:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.288 4322021569875434240 294.62436862781 +17.23719604953 12.9166 12.3421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265422_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265422_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:51:31.18 +15:42:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.640 1819784931914167552 297.88033920958 +15.70502869303 12.7461 12.2637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265481_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265481_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:47.37 +12:55:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.956 4317001410293765120 294.44686478519 +12.92006898009 13.0720 12.6366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265484_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265484_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:52:34.01 +15:56:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265521_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265521_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:57:32.28 +16:11:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265615_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265615_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:07:06.89 +15:13:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265654_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265654_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:55:10.32 +13:10:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.220 4305053562843867904 298.79437414350 +13.18241334417 12.2640 11.2994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265686_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 265686_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:30:28.70 +11:34:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.685 4314979270978573056 292.61830777551 +11.56656208138 13.4865 12.5560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81905_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 81905_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:39:45.99 +12:39:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231076_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 231076_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:47.50 +17:41:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246140_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 246140_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:25:26.43 +10:11:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 5.759 4308733696981840000 291.35935533192 +10.19813109437 11.9530 10.5647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246080_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 246080_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:47:11.25 +14:28:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.395 4317497564894148224 296.79717319778 +14.48065049892 12.6268 11.7268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228052_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 228052_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 232576_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 232576_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 59392_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 59392_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:27:20.27 +11:39:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 4.703 4315722643888130048 291.83465126140 +11.65632047266 11.1677 9.5977 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34767_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 34767_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:38:25.65 +10:35:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152514_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
Preparing report for the candidate 152514_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
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Considering the candidate 59017_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 59017_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:28:46.72 +11:38:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116431_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 116431_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:30.21 +14:00:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67015_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 67015_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:50:19.55 +12:05:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22086_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 22086_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:47:35.95 +09:56:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53842_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 53842_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:48:22.98 +11:31:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42572_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 42572_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:36:28.29 +10:58:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22571_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 22571_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:40:43.07 +09:55:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128316_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 128316_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:36:15.58 +14:23:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 125694_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 125694_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:27:33.92 +14:16:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134116_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 134116_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:22.35 +14:35:46.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113337_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 113337_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:41:05.48 +13:48:58.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99938_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 99938_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:44:34.10 +13:18:11.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95567_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 95567_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:24.27 +13:01:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72686_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 72686_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:42:12.77 +12:11:37.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50919_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 50919_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:36:52.44 +11:16:26.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179324_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 179324_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:17.29 +16:27:48.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179878_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 179878_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:39:25.22 +16:34:16.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70242_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 70242_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:24:59.61 +11:56:59.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63739_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 63739_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:42:33.97 +11:49:38.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25300_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 25300_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:22:48.39 +09:54:51.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80728_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 80728_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:39.48 +12:22:32.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183563_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 183563_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:41:02.96 +17:28:32.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59306_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 59306_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:53.18 +11:32:08.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62827_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 62827_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:48:42.02 +11:48:59.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135660_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 135660_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:16:26.89 +14:32:43.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221600_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 221600_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:40:05.83 +18:00:48.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38760_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 38760_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:46:15.34 +10:36:54.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149148_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 149148_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:20.29 +15:05:02.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62138_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 62138_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:49.12 +11:35:47.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181140_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 181140_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:56:01.22 +16:38:06.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187320_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 187320_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:57:45.55 +16:47:24.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123650_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 123650_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:24.68 +13:51:49.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51844_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 51844_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks
**** FOUND 19:06:58.57 +11:04:18.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32529_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412
The candidate 32529_fd_Aql-01-Q2b1x1_2026-03-27_04-24-41_20.00sec_-15.00C_LIGHT_0412 did not pass the final checks