This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa
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 4303291084369220608,2461128.8713,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4303291084369220608 20260329.3713 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:40.26 +10:19:56.0 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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 4304819542989148160,2461128.8713,12.64,0.05,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 4304819542989148160 20260329.3713 12.64CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:39.71 +12:36:44.1 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195708.73+134750.6,2461128.8713,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195708.73+134750.6 20260329.3713 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:08.74 +13:47:42.8 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194542.97+174418.7,2461128.8713,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194542.97+174418.7 20260329.3713 12.98CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:42.79 +17:44:15.4 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
V0827 Aql,2461128.8713,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0827 Aql 20260329.3713 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:50.52 +10:49:38.7 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3713 2461128.8713 11.00 19:57:22.15 +13:56:34.2
53.00145 -7.77038 galactic Aql Second-epoch detections are separated by 0.9" and 8.5 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 1807156388019136000 | 19:57:22.08 +13:56:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1807156388019136000,2461128.8713,11.00,0.05,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 1807156388019136000 20260329.3713 11.00CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:22.15 +13:56:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
Mis V0921,2461128.8713,11.76,0.05,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
Mis V0921 20260329.3713 11.76CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:46.69 +11:38:30.8 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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 J192203.06+094244.9,2461128.8713,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192203.06+094244.9 20260329.3713 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:03.08 +09:42:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3713 2461128.8713 12.66 19:55:46.96 +12:59:18.2
51.97346 -7.92099 galactic Aql Second-epoch detections are separated by 2.5" and 8.3 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 4305034115231901184 | 19:55:46.99 +12:59:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.847+/-0.028 (M)
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 4305034115231901184,2461128.8713,12.66,0.05,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 4305034115231901184 20260329.3713 12.66CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:46.96 +12:59:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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 J192517.60+102802.5,2461128.8713,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192517.60+102802.5 20260329.3713 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:25:18.23 +10:28:15.3 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3713 2461128.8713 12.52 19:55:05.48 +12:50:29.8
51.75976 -7.84948 galactic Aql Second-epoch detections are separated by 2.0" and 8.5 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 4305026800918060288 | 19:55:04.06 +12:50:46.0 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE
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 4305026800918060288,2461128.8713,12.52,0.05,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 4305026800918060288 20260329.3713 12.52CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:05.48 +12:50:29.8 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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 V449,2461128.8713,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V449 20260329.3713 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:50.14 +17:51:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
V0677 Aql,2461128.8713,11.96,0.05,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
V0677 Aql 20260329.3713 11.96CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:30.58 +10:04:05.5 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
OX Aql,2461128.8713,10.83,0.05,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
OX Aql 20260329.3713 10.83CV 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/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:24.74 +15:06:40.7 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193816.55+103659.6,2461128.8713,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193816.55+103659.6 20260329.3713 12.27CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:16.31 +10:36:55.1 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
V1543 Aql,2461128.8713,12.65,0.05,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
V1543 Aql 20260329.3713 12.65CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:14.91 +10:35:41.5 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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 J193604+1032.5,2461128.8713,12.10,0.05,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 J193604+1032.5 20260329.3713 12.10CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:04.45 +10:32:22.7 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195743.52+150106.6,2461128.8713,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195743.52+150106.6 20260329.3713 12.12CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:43.19 +15:01:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194830.04+103358.5,2461128.8713,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194830.04+103358.5 20260329.3713 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:48:29.93 +10:33:59.0 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3713 2461128.8713 12.76 19:49:11.95 +09:57:49.7
48.51403 -8.03008 galactic Aql Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.3020+09.9638 | 19:49:12.09 +09:57:51.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.3020+09.9638,2461128.8713,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.3020+09.9638 20260329.3713 12.76CV 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:11.95 +09:57:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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
MU Aql,2461128.8713,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MU Aql 20260329.3713 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:11.57 +13:20:24.5 ;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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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_2026-03-29_03-54-53_20_00sec_-15_00C_LIGHT_0326_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_2026-03-29_03-53-59_20_00sec_-14_90C_LIGHT_0325_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: 2461128.87157098 29.03.2026 08:54:53.733 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 4 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): 16827
Objects passed selection criteria: 16768
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 13202.8
Average stars matched: 12812.8 (97.0461 %)
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 Sun Mar 29 03:56:59 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: 2461128.87157098 29.03.2026 08:54:53.733 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 141
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: 41 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): 183222
Objects passed selection criteria: 182771
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 138000
Average stars matched: 132382 (95.9293 %)
Memory usage VmPeak: 2148676 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 04:01:39 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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461128.87094899
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits'
wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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 19:33:21.678 +13:55:23.20
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:24.068 +13:55:58.26
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:21.678 +13:55:23.20
Second-epoch second image center 19:33:24.068 +13:55:58.26
Angular distance between the image centers 0.01372 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.es2YHg6Wxu
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.zcSKRZRmdH
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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits &> /tmp/tmp.aC2pXXh8yR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits &> /tmp/tmp.S0AcHyFQO4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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 3 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
2.9 pix fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
2.8 pix fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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
13.8 mag. fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
13.8 mag. fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.es2YHg6Wxu (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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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.zcSKRZRmdH (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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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.aC2pXXh8yR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=524, passed=9548
Got 9548 stars (including 9020 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat
util/solve_plate_with_UCAC5 got 9548 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.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.S0AcHyFQO4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=9524
Got 9524 stars (including 8956 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 9524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.82"
Estimated accuracy of the plate solution: 0.91"
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_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits'
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out03088.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31516_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 31516_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:40:42.93 +09:55:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03088_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 03088_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08916_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 08916_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:53:50.13 +13:09:25.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
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 ####
19:50:40.26 +10:19:56.0
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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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 19:33:21.678 +13:55:23.20
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:24.068 +13:55:58.26
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:21.678 +13:55:23.20
Second-epoch second image center 19:33:24.068 +13:55:58.26
Angular distance between the image centers 0.01372 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.sQWzCWvC4l
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.ONDFBvdDs3
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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits &> /tmp/tmp.qiuHKXw5QX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits &> /tmp/tmp.ZuNQprXavn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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 111 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
2.8 pix fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
2.5 pix fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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
13.8 mag. fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
13.9 mag. fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
All-image limiting magnitude estimate: 13.8 (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.sQWzCWvC4l (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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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.ONDFBvdDs3 (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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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.qiuHKXw5QX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5948, passed=77377
Got 77377 stars (including 71364 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat
util/solve_plate_with_UCAC5 got 77377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.75"
Estimated accuracy of the plate solution: 0.83"
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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.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.ZuNQprXavn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=6254, passed=82320
Got 82320 stars (including 75984 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 82320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.75"
Estimated accuracy of the plate solution: 0.84"
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_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/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_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-53-59_20.00sec_-14.90C_LIGHT_0325.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-01-Q2b1x1_035532_TTUQ2b1x1_15052_4UFsZyDa/wcs_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326.fits
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out154623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out233003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265012.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__out265022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out265600.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out113313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out228832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99078.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 9s
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Considering the candidate 264967_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264967_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:30:38.35 +12:36:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 264976_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264976_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:43:34.93 +16:22:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264979_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264979_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:40:48.80 +15:00:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 264981_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264981_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:11:37.59 +16:51:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 264984_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264984_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:40:52.42 +12:38:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.801 4316783260307254144 295.21892786660 +12.64315585283 13.0726 12.6907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 264986_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264986_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:56:23.61 +12:40:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264989_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264989_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:45:29.41 +12:49:35.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 264994_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264994_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:28:32.48 +15:56:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264998_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 264998_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:42:29.26 +17:24:15.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 265002_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265002_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:37:43.60 +11:29:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265005_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265005_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:45:43.65 +14:57:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)
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Considering the candidate 265009_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265009_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:07:39.89 +17:48:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.667 4514408483850933760 286.91572525245 +17.80682562040 13.1550 12.2862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265010_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265010_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:31:07.61 +11:31:33.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 265012_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265012_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:43:28.71 +11:23:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 265016_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265016_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:53:16.73 +15:55:19.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 265017_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265017_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:54:12.93 +12:16:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.795 4304161485267048192 298.55384388404 +12.27333147657 12.3341 11.4486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265020_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 265020_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 265022_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265022_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:42:35.72 +11:47:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.765 4304668428863439360 295.64759819076 +11.78532252947 12.9042 12.3417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265023_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265023_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:49:08.28 +11:41:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.551 4304476976388944640 297.28486223301 +11.69457960532 12.4240 11.9922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265024_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265024_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:57:45.52 +13:01:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.354 4304310950130530560 299.44005228525 +13.02901462804 12.0565 11.2719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265025_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265025_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:41:26.26 +10:00:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265026_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265026_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:51:17.87 +16:24:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.189 1819973974860248064 297.82486313307 +16.40940720495 12.3496 11.5348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265028_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265028_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:51:56.11 +16:11:38.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 265030_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265030_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:51:34.02 +12:46:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)
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Considering the candidate 265031_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265031_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:40:47.63 +18:05:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.838 1824096220119757824 295.19894582945 +18.09908455817 12.6338 11.7389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265035_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265035_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:56:27.91 +13:04:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.618 4305059442670597888 299.11593502509 +13.07833191147 12.0128 11.5438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265036_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265036_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 265037_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265037_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:58:07.85 +12:10:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265038_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265038_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:54:49.93 +13:55:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.809 4305351672250385664 298.70797910512 +13.91991734671 11.8974 11.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265040_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265040_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:51:21.28 +09:54:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.423 4303213362638995328 297.83921362565 +09.91648676428 11.6785 11.0830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265043_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265043_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:53:21.91 +12:54:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 4.235 4304994468411228416 298.34071220933 +12.90505971341 11.7904 11.4654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265048_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265048_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:56:44.10 +12:05:20.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 265312_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265312_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:37:50.90 +12:47:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265415_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265415_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:18:28.14 +15:30:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.003 4320777373749479424 289.61710448663 +15.51421301051 11.7107 10.4313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265430_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265430_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:42:37.03 +11:47:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.567 4304667668622283392 295.65461065771 +11.78438663092 12.1244 11.2143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265436_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265436_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:57:32.17 +16:11:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265441_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265441_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:08:24.85 +13:04:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.635 4314102131225507840 287.10318925772 +13.07663077470 12.6004 11.8380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265453_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265453_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:36:10.02 +12:08:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.839 4315248685677483264 294.04283896781 +12.14161769457 12.6586 11.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265457_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265457_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:13:27.96 +14:36:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.597 4320502869446941056 288.36746910535 +14.61526149224 12.7253 12.0112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265458_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265458_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:23:09.45 +14:53:55.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265461_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265461_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:37:23.33 +16:27:01.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265483_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265483_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:37:10.36 +16:27:59.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265489_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265489_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:36:08.95 +12:08:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.889 4315248307720360832 294.03754974857 +12.13773808560 12.1916 11.0535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265533_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265533_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:16:20.46 +14:31:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265538_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265538_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:52:49.41 +16:14:30.2 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 265540_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265540_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:38:29.53 +17:14:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265546_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265546_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:07:06.72 +15:13:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265563_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265563_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:09:38.69 +11:06:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.323 4312464172464952448 287.41180699262 +11.11626687864 12.6685 11.5810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265570_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265570_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:19:20.84 +14:11:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.193 4319494003123699328 289.83757182984 +14.19005777263 12.8788 12.2581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265575_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265575_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:18:34.22 +16:42:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.066 4321196253290842880 289.64314397699 +16.71060532741 13.1047 12.3630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265576_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265576_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:05:14.77 +13:52:39.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 265580_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265580_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:55:10.35 +13:10:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265595_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265595_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:51:31.23 +15:42:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265596_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265596_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:31:20.79 +11:37:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.043 4314939310602005760 292.83587599220 +11.62007246783 13.2662 12.9754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265600_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265600_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:41:10.00 +13:27:48.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 265603_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 265603_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 265607_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265607_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:41:28.55 +17:09:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.628 1823962045324188800 295.36995908056 +17.15284879351 12.8246 11.8862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265656_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265656_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:37:47.27 +12:55:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265657_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265657_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:35:31.44 +15:37:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.471 4318388134963092480 293.88122266182 +15.62704228034 12.9116 12.3260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265659_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265659_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:50:10.89 +15:34:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265690_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265690_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:32:03.09 +11:43:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265727_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265727_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:15:11.51 +10:14:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265732_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265732_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:09:47.81 +16:00:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.964 4512874046672995072 287.44916212734 +16.00576176414 13.1651 12.1819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265744_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265744_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:28:53.45 +15:14:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.837 4321304039775714048 292.22239354151 +15.23867152660 12.8420 11.8033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265759_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265759_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:26:19.04 +16:40:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265762_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265762_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:08:59.56 +13:08:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.920 4314103441258092800 287.24722434624 +13.14116943079 13.3129 10.7689 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 265794_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 265794_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:24:43.72 +16:56:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.819 4322563251152869888 291.18234333695 +16.93700402429 13.1773 11.9470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 249271_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 249271_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:55:47.24 +13:27:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72838_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 72838_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:43:21.82 +12:19:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.199 4304722133137845120 295.84160309564 +12.32030504392 11.8915 10.0165 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82444_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 82444_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:55:54.23 +12:42:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233003_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 233003_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:43:30.42 +17:39:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.135 1824009289970656256 295.87715981113 +17.66163952694 11.2446 9.7759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81905_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 81905_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:39:45.78 +12:39:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30144_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 30144_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:50:40.25 +10:19:55.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 232202_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 232202_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 68230_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 68230_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:55:17.48 +12:08:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231076_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 231076_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:29:47.03 +17:41:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228052_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 228052_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:06:01.03 +17:34:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39344_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 39344_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 113313_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 113313_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 154623_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 154623_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:34:59.16 +15:36:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.995 4321389011421283328 293.74585116826 +15.61163254506 10.3516 8.7456 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59017_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 59017_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 232576_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 232576_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:05:29.94 +17:20:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20126_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 20126_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 89577_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 89577_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 152514_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 152514_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:33:40.56 +15:31:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34085_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 34085_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 86090_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 86090_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 59392_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 59392_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:27:20.19 +11:39:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228832_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 228832_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 24513_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 24513_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 34767_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 34767_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:38:25.53 +10:35:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142666_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 142666_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 35297_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 35297_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 34250_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 34250_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 94039_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 94039_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:53:50.12 +13:09:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37298_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 37298_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 85689_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 85689_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:50:40.50 +12:49:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104006_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 104006_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:55:16.57 +13:33:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139698_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 139698_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 33590_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 33590_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 116431_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 116431_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:29:30.16 +14:00:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67015_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 67015_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:50:19.35 +12:05:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22382_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 22382_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 22086_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 22086_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:47:35.76 +09:56:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65772_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 65772_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:32:22.85 +11:59:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53842_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 53842_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:48:22.87 +11:31:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99078_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
Preparing report for the candidate 99078_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
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Considering the candidate 124059_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 124059_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:58:34.36 +14:23:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22571_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 22571_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:40:42.93 +09:55:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246383_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 246383_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks
**** FOUND 19:47:36.27 +13:08:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.115 4305248142041564288 296.90125061174 +13.14024317913 11.8772 10.5221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42572_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326
The candidate 42572_fd_Aql-01-Q2b1x1_2026-03-29_03-54-53_20.00sec_-15.00C_LIGHT_0326 did not pass the final checks