This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1
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
target,2461126.9471,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4471 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:54.68 +12:56:18.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J193107.90+172927.5,2461126.9471,13.40,0.05,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 J193107.90+172927.5 20260327.4471 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:07.49 +17:29:32.2 ;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_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J193916.20+120622.6,2461126.9471,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193916.20+120622.6 20260327.4471 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:16.89 +12:06:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J193625.55+165547.5,2461126.9471,13.17,0.05,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 J193625.55+165547.5 20260327.4471 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:25.89 +16:55:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9471,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4471 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:12:38.75 +11:09:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.99 19:40:28.55 +15:19:50.9
52.15886 -3.53719 galactic Aql Second-epoch detections are separated by 5.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J194026.26+151918.1 | 19:40:26.26 +15:19:18.0 (Gaia DR3) | SRS (local) | 25.964000000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194026.26+151918.1,2461126.9471,12.99,0.05,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 J194026.26+151918.1 20260327.4471 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:28.55 +15:19:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J195037.39+180533.2,2461126.9471,12.96,0.05,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
ZTF J195037.39+180533.2 20260327.4471 12.96CV 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/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:36.98 +18:05:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 13.04 19:30:10.22 +10:50:02.2
46.99980 -3.51550 galactic Aql Second-epoch detections are separated by 0.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.5395+10.8328 | 19:30:09.50 +10:49:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.5395+10.8328,2461126.9471,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.5395+10.8328 20260327.4471 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:30:10.22 +10:50:02.2 ;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_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J191721.37+155339.5,2461126.9471,12.68,0.05,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
ZTF J191721.37+155339.5 20260327.4471 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/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:17:20.24 +15:53:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J192947.07+174138.8,2461126.9471,12.97,0.05,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 J192947.07+174138.8 20260327.4471 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:47.28 +17:41:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.84 19:33:21.93 +11:49:46.7
48.25141 -3.72653 galactic Aql Second-epoch detections are separated by 3.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4315309811668002176 | 19:33:21.49 +11:49:13.8 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4315309811668002176,2461126.9471,12.84,0.05,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 4315309811668002176 20260327.4471 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:21.93 +11:49:46.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.71 19:31:35.61 +11:29:18.2
47.74289 -3.50947 galactic Aql Second-epoch detections are separated by 1.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.8930+11.4821 | 19:31:35.61 +11:29:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.8930+11.4821,2461126.9471,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.8930+11.4821 20260327.4471 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:35.61 +11:29:18.2 ;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_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 13.15 19:43:56.92 +13:45:35.2
51.20158 -5.04156 galactic Aql Second-epoch detections are separated by 1.7" and 4.3 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 | ATO J295.9859+13.7564 | 19:43:56.92 +13:45:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.9859+13.7564,2461126.9471,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.9859+13.7564 20260327.4471 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:56.92 +13:45:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 4313972835527633792,2461126.9471,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4313972835527633792 20260327.4471 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_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:33.47 +12:44:18.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9471,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4471 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:05:39.29 +11:36:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.72 19:45:47.30 +15:46:17.0
53.17633 -4.43218 galactic Aql Second-epoch detections are separated by 2.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.4469+15.7749 | 19:45:47.30 +15:46:17.0 (user input) | STOCH (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.4469+15.7749,2461126.9471,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.4469+15.7749 20260327.4471 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:47.30 +15:46:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.61 19:19:44.17 +16:01:54.0
50.37904 1.17921 galactic Aql Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4321075444446080384 | 19:19:43.70 +16:01:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4321075444446080384,2461126.9471,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4321075444446080384 20260327.4471 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:44.17 +16:01:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 4320727620812445056,2461126.9471,12.52,0.05,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 4320727620812445056 20260327.4471 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_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:11.62 +15:10:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4471 2461126.9471 12.47 19:10:05.50 +11:40:32.4
45.43331 1.22720 galactic Aql Second-epoch detections are separated by 2.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4313061031145380096 | 19:10:05.95 +11:40:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4313061031145380096,2461126.9471,12.47,0.05,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 4313061031145380096 20260327.4471 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:10:05.50 +11:40:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 J190501.57+173232.1,2461126.9471,12.51,0.05,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 J190501.57+173232.1 20260327.4471 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:05:01.17 +17:32:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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 1807299427605945856,2461126.9471,12.60,0.05,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
Gaia DR3 1807299427605945856 20260327.4471 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_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:34.43 +14:23:11.2 ;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_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_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
LO Aql,2461126.9471,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LO Aql 20260327.4471 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:27.87 +10:58:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461126.94740472 27.03.2026 10:44:05.768 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 30
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: 7 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): 17794
Objects passed selection criteria: 17784
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 16500.5
Average stars matched: 15988.8 (96.8986 %)
Memory usage VmPeak: 123236 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:33:52 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461126.94740472 27.03.2026 10:44:05.768 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 184
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: 80 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): 183925
Objects passed selection criteria: 183532
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: 146675
Average stars matched: 140862 (96.0363 %)
Memory usage VmPeak: 2672964 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:37:57 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.94688354
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits'
wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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 19:33:25.328 +13:57:49.41
Angular distance between the image centers 0.04 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 19:33:25.142 +13:57:27.34
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:25.328 +13:57:49.41
Second-epoch second image center 19:33:25.142 +13:57:27.34
Angular distance between the image centers 0.00618 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.4ELE2c1HPF
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.EdHzx9h0LL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits &> /tmp/tmp.Zu4HfIsMhr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.R5Rw2bDMQR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.2 pix Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
3.2 pix fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
4.2 pix fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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
14.4 mag. fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
14.2 mag. fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (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.4ELE2c1HPF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/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.EdHzx9h0LL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/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.Zu4HfIsMhr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1359, passed=19928
Got 19928 stars (including 18548 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat
util/solve_plate_with_UCAC5 got 19928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.66"
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_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.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.R5Rw2bDMQR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=985, passed=15988
Got 15988 stars (including 15001 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 15988 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits'
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31735.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31539_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31539_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:40:43.04 +09:55:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31579_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31579_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:37:30.23 +12:40:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31595_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31595_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31614_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31614_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:50:40.71 +12:49:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31617_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31617_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:37:11.50 +13:08:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31621_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31621_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:26:27.72 +13:10:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31623_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31623_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:33:42.87 +13:01:16.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31624_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31624_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:33:37.86 +12:48:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31625_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31625_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:20:06.07 +11:58:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31628_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31628_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:33:22.20 +13:38:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31636_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31636_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:31:04.06 +13:15:28.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31637_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31637_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:23:20.02 +13:51:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31638_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31638_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:40:53.82 +13:01:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31640_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31640_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:25:53.38 +12:50:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31643_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31643_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:25:31.75 +13:28:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31644_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31644_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:31:24.33 +12:39:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31649_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31649_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:31:32.74 +12:32:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31652_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31652_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:29:19.78 +12:40:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31654_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31654_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:29:39.48 +12:48:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31658_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31658_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:30:02.68 +11:14:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31664_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31664_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:28:33.39 +13:27:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31673_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31673_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:39:37.87 +12:43:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.607 4316798580405849216 294.90704976337 +12.72849525729 11.8827 11.6915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31674_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31674_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:38:07.51 +11:07:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31681_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31681_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:22:28.48 +13:47:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31684_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31684_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:32:21.06 +12:06:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.383 4315379424504814976 293.08755607522 +12.11355488350 11.7990 11.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31709_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31709_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:12:34.68 +11:49:03.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31735_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 31735_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:26:52.58 +14:37:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.705 4319766200968323072 291.71909746420 +14.62255675955 11.7141 11.2126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Creating symlink local_wcs_cache/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits exists and is non-empty
wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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 19:33:25.328 +13:57:49.41
Angular distance between the image centers 0.04 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 19:33:25.142 +13:57:27.34
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:25.328 +13:57:49.41
Second-epoch second image center 19:33:25.142 +13:57:27.34
Angular distance between the image centers 0.00618 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.OlATcSiDYR
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.Rm0kVukLkh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits &> /tmp/tmp.iNKM0ZW3Pf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits &> /tmp/tmp.2CNW2b7Kjj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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 104 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.0 pix Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
3.3 pix fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
4.5 pix fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.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
14.5 mag. fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
14.2 mag. fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.3 (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.OlATcSiDYR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/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.Rm0kVukLkh (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/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.iNKM0ZW3Pf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=20124, passed=128006
Got 128006 stars (including 107782 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat
util/solve_plate_with_UCAC5 got 128006 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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: 0.62"
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 969 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: 0.65"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.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.2CNW2b7Kjj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Checking if the catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat corresponding to the image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
WCS catalog name: wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=14168, passed=85979
Got 85979 stars (including 71773 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 85979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.81"
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_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits -region wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Saving fully-calibrated image wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_Aql-01-Q2b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-43-20_20.00sec_-15.00C_LIGHT_0501.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Aql-01-Q2b1x1_072942_TTUQ2b1x1_20824_pgiFTZs1/wcs_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502.fits
Preparing the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out246251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out108905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out228869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90319.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 11s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264971_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 264971_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264997_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 264997_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264998_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 264998_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:06:14.78 +14:56:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.946 4512680807499223552 286.56186669102 +14.94024388994 13.0846 12.4398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265018_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265018_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265028_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265028_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:44:52.16 +15:02:05.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265034_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265034_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265048_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265048_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:46:24.75 +17:18:41.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265053_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265053_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:08:15.14 +17:59:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.902 4514418306391748608 287.06224155706 +17.99984965070 12.7296 11.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265055_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265055_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:46:03.11 +17:30:21.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265060_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265060_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:54:21.30 +16:15:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265061_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265061_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:41:29.87 +15:56:52.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265075_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265075_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:46:54.51 +16:11:23.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265079_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265079_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265088_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265088_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265093_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265093_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:44:18.41 +15:39:14.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265103_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265103_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265114_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265114_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265125_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265125_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265128_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265128_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265143_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265143_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:09:14.90 +14:42:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265145_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265145_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265147_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265147_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:55:48.28 +12:53:00.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265150_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265150_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:31:00.46 +12:47:08.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265155_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 265155_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265159_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265159_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:32:10.25 +12:33:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.563 4316182171015569792 293.04237485001 +12.56028736882 10.4030 8.9395 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265410_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265410_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265533_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265533_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:37:51.02 +12:47:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265588_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265588_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265663_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265663_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265726_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265726_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265763_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265763_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265773_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265773_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265904_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265904_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265933_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265933_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:07:06.95 +15:13:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265946_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265946_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265972_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265972_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265975_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265975_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265996_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 265996_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266005_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266005_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266032_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266032_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266073_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266073_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266101_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266101_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266115_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266115_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266128_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266128_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266137_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266137_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266157_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266157_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266176_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266176_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266189_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266189_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266220_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266220_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266245_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266245_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266287_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266287_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266333_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266333_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266354_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266354_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266361_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266361_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266417_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266417_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266424_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266424_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266446_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266446_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266468_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266468_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266472_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266472_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266477_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266477_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266478_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266478_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266492_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 266492_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246068_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 246068_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231076_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 231076_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196020_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 196020_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:05:55.93 +16:43:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246251_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 246251_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:41:32.53 +11:17:07.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246080_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 246080_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:47:11.30 +14:28:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61758_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 61758_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54172_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 54172_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108905_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 108905_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228052_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 228052_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:06:01.15 +17:34:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59017_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 59017_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:28:46.74 +11:38:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90319_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 90319_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159883_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 159883_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81905_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 81905_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:39:46.11 +12:39:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62121_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 62121_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181287_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 181287_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:05:10.26 +16:26:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232576_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 232576_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:05:29.86 +17:20:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34767_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 34767_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:38:25.60 +10:35:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157366_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 157366_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167574_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 167574_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134109_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 134109_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172572_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 172572_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67015_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 67015_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:50:19.69 +12:05:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147111_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 147111_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185617_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 185617_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:26:17.56 +17:28:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116431_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 116431_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:29:30.36 +14:00:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22086_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 22086_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:47:35.85 +09:56:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62640_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 62640_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22571_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 22571_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:40:43.03 +09:55:54.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65772_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 65772_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:32:23.13 +11:59:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228869_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 228869_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124059_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 124059_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42572_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
Preparing report for the candidate 42572_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125694_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 125694_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:27:33.94 +14:16:59.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113337_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 113337_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:41:05.54 +13:48:59.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95567_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 95567_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:26:24.30 +13:01:30.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179324_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 179324_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:37:17.32 +16:27:49.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179878_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 179878_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:39:25.29 +16:34:16.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195750_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 195750_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:24:22.14 +16:56:16.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59306_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 59306_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:19:53.22 +11:32:09.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135660_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 135660_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:16:26.93 +14:32:43.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149148_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 149148_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:15:20.31 +15:05:03.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193832_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502
The candidate 193832_fd_Aql-01-Q2b1x1_2026-03-27_05-44-05_20.00sec_-15.00C_LIGHT_0502 did not pass the final checks
**** FOUND 19:07:57.56 +16:51:05.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 45s
Prepared the HTML report for the field Aql-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:43:56.92 +13:45:35.2
19:58:34.43 +14:23:11.2
19:18:11.62 +15:10:35.2
19:45:47.30 +15:46:17.0
19:19:44.17 +16:01:54.0
19:05:01.17 +17:32:18.8
19:29:47.28 +17:41:34.5
19:40:54.68 +12:56:18.4
19:31:07.49 +17:29:32.2
19:39:16.89 +12:06:25.6
19:36:25.89 +16:55:54.6
19:12:38.75 +11:09:55.4
19:40:28.55 +15:19:50.9
19:50:36.98 +18:05:43.0
19:30:10.22 +10:50:02.2
19:17:20.24 +15:53:49.0
19:36:27.87 +10:58:14.7
19:31:35.61 +11:29:18.2
19:33:21.93 +11:49:46.7
19:05:39.29 +11:36:12.7
19:10:05.50 +11:40:32.4
19:06:33.47 +12:44:18.9
########### Completed Aql-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:40:54.68 +12:56:18.4
19:31:07.49 +17:29:32.2
19:39:16.89 +12:06:25.6
19:36:25.89 +16:55:54.6
19:12:38.75 +11:09:55.4
19:40:28.55 +15:19:50.9
19:50:36.98 +18:05:43.0
19:30:10.22 +10:50:02.2
19:17:20.24 +15:53:49.0
19:29:47.28 +17:41:34.5
19:33:21.93 +11:49:46.7
19:31:35.61 +11:29:18.2
19:43:56.92 +13:45:35.2
19:06:33.47 +12:44:18.9
19:05:39.29 +11:36:12.7
19:45:47.30 +15:46:17.0
19:19:44.17 +16:01:54.0
19:18:11.62 +15:10:35.2
19:10:05.50 +11:40:32.4
19:05:01.17 +17:32:18.8
19:58:34.43 +14:23:11.2
19:36:27.87 +10:58:14.7
###################################################################################
19:40:54.68 +12:56:18.4 -- not an asteroid (will add it to exclusion list)
19:31:07.49 +17:29:32.2 -- not an asteroid (will add it to exclusion list)
19:39:16.89 +12:06:25.6 -- not an asteroid (will add it to exclusion list)
19:36:25.89 +16:55:54.6 -- not an asteroid (will add it to exclusion list)
19:12:38.75 +11:09:55.4 -- not an asteroid (will add it to exclusion list)
19:40:28.55 +15:19:50.9 -- not an asteroid (will add it to exclusion list)
19:50:36.98 +18:05:43.0 -- not an asteroid (will add it to exclusion list)
19:30:10.22 +10:50:02.2 -- not an asteroid (will add it to exclusion list)
19:17:20.24 +15:53:49.0 -- not an asteroid (will add it to exclusion list)
19:29:47.28 +17:41:34.5 -- not an asteroid (will add it to exclusion list)
19:33:21.93 +11:49:46.7 -- not an asteroid (will add it to exclusion list)
19:31:35.61 +11:29:18.2 -- not an asteroid (will add it to exclusion list)
19:43:56.92 +13:45:35.2 -- not an asteroid (will add it to exclusion list)
19:06:33.47 +12:44:18.9 -- not an asteroid (will add it to exclusion list)
19:05:39.29 +11:36:12.7 -- not an asteroid (will add it to exclusion list)
19:45:47.30 +15:46:17.0 -- not an asteroid (will add it to exclusion list)
19:19:44.17 +16:01:54.0 -- not an asteroid (will add it to exclusion list)
19:18:11.62 +15:10:35.2 -- not an asteroid (will add it to exclusion list)
19:10:05.50 +11:40:32.4 -- not an asteroid (will add it to exclusion list)
19:05:01.17 +17:32:18.8 -- not an asteroid (will add it to exclusion list)
19:58:34.43 +14:23:11.2 -- not an asteroid (will add it to exclusion list)
19:36:27.87 +10:58:14.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:05:01.17 +17:32:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:39.29 +11:36:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:33.47 +12:44:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:05.50 +11:40:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:38.75 +11:09:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:20.24 +15:53:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:18:11.62 +15:10:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:44.17 +16:01:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:47.28 +17:41:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:10.22 +10:50:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:07.49 +17:29:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:35.61 +11:29:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:21.93 +11:49:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:25.89 +16:55:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:27.87 +10:58:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:16.89 +12:06:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:28.55 +15:19:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:54.68 +12:56:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:56.92 +13:45:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:47.30 +15:46:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:36.98 +18:05:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:34.43 +14:23:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:05:01.17 +17:32:18.8 -- a known variable star
19:05:39.29 +11:36:12.7 -- not a known variable star
19:06:33.47 +12:44:18.9 -- a known variable star
19:10:05.50 +11:40:32.4 -- not a known variable star
19:12:38.75 +11:09:55.4 -- not a known variable star
19:17:20.24 +15:53:49.0 -- a known variable star
19:18:11.62 +15:10:35.2 -- a known variable star
19:19:44.17 +16:01:54.0 -- not a known variable star
19:29:47.28 +17:41:34.5 -- a known variable star
19:30:10.22 +10:50:02.2 -- not a known variable star
19:31:07.49 +17:29:32.2 -- a known variable star
19:31:35.61 +11:29:18.2 -- not a known variable star
19:33:21.93 +11:49:46.7 -- not a known variable star
19:36:25.89 +16:55:54.6 -- a known variable star
19:36:27.87 +10:58:14.7 -- a known variable star
19:39:16.89 +12:06:25.6 -- a known variable star
19:40:28.55 +15:19:50.9 -- not a known variable star
19:40:54.68 +12:56:18.4 -- not a known variable star
19:43:56.92 +13:45:35.2 -- not a known variable star
19:45:47.30 +15:46:17.0 -- not a known variable star
19:50:36.98 +18:05:43.0 -- a known variable star
19:58:34.43 +14:23:11.2 -- a known variable star
Found 11 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
22 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:05:01.17 +17:32:18.8
19:05:39.29 +11:36:12.7
19:06:33.47 +12:44:18.9
19:10:05.50 +11:40:32.4
19:12:38.75 +11:09:55.4
19:17:20.24 +15:53:49.0
19:18:11.62 +15:10:35.2
19:19:44.17 +16:01:54.0
19:29:47.28 +17:41:34.5
19:30:10.22 +10:50:02.2
19:31:07.49 +17:29:32.2
19:31:35.61 +11:29:18.2
19:33:21.93 +11:49:46.7
19:36:25.89 +16:55:54.6
19:36:27.87 +10:58:14.7
19:39:16.89 +12:06:25.6
19:40:28.55 +15:19:50.9
19:40:54.68 +12:56:18.4
19:43:56.92 +13:45:35.2
19:45:47.30 +15:46:17.0
19:50:36.98 +18:05:43.0
19:58:34.43 +14:23:11.2
19:39:37.87 +12:43:42.5
19:32:21.06 +12:06:50.0
19:26:52.58 +14:37:19.5
19:41:32.53 +11:17:07.1
19:06:14.78 +14:56:23.2
19:44:52.16 +15:02:05.9
19:46:24.75 +17:18:41.3
19:08:15.14 +17:59:59.8
19:46:03.11 +17:30:21.6
19:54:21.30 +16:15:04.0
19:41:29.87 +15:56:52.1
19:46:54.51 +16:11:23.6
19:44:18.41 +15:39:14.4
19:31:00.46 +12:47:08.6
19:32:10.25 +12:33:36.0
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461126.94688354 -observatory 500
22:47:14.97 -08:14:34.0 Mercury (0.6mag)
01:36:04.33 +09:20:08.4 Venus (-3.9mag)
23:21:53.82 -05:15:15.6 Mars (1.2mag)
07:05:55.74 +22:56:29.6 Jupiter (-2.2mag)
00:20:18.25 -00:07:09.3 Saturn (0.9mag)
03:43:58.00 +19:35:19.1 Uranus (5.8mag)
00:08:11.21 -00:32:15.4 Neptune (7.8mag)
20:32:32.91 -22:53:03.6 Pluto (14.5mag)
08:01:53.77 +23:58:24.2 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Mar 27 07:33 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461126.94688354:
07:05:51.00 +22:56:40.8 Io (5.6mag)
07:05:52.90 +22:56:31.7 Europa (5.8mag)
07:05:43.58 +22:56:46.0 Ganymede (5.2mag)
07:06:12.51 +22:56:07.6 Callisto (6.5mag)
07:09:53.20 +22:54:22.5 Himalia (15.2mag)
07:05:57.48 +22:56:23.8 Thebe (16.1mag)
07:09:36.60 +23:20:16.2 Elara (17.2mag)
07:03:29.19 +23:46:45.8 Pasiphae (17.3mag)
07:14:37.60 +22:52:03.2 Carme (18.4mag)
00:20:29.95 -00:07:06.1 Titan (8.8mag)
00:20:18.04 -00:06:53.8 Rhea (10.1mag)
00:20:39.48 -00:04:57.5 Iapetus (11.5mag)
00:20:19.68 -00:06:45.3 Hyperion (14.8mag)
00:22:08.77 +00:03:34.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 27 07:33 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461126.94688354:
13:40:46.43 +01:50:01.7 JWST
18:13:51.43 +31:21:51.8 Chandra
09:08:32.39 -49:18:00.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 27 07:33 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461126.94688354 -observatory 500
18:40:34.60 -27:45:16.1 14.0mag P/2010 H2 (Vales)
04:54:23.01 -70:40:14.4 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:15.77 +31:19:34.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:28.68 +08:11:05.3 17.6mag C/2021 G2 (ATLAS)
23:04:00.03 +28:34:48.7 17.0mag C/2022 E2 (ATLAS)
04:07:16.97 +25:28:54.2 15.8mag C/2022 N2 (PANSTARRS)
09:01:29.83 +31:40:29.5 16.1mag C/2022 QE78 (ATLAS)
08:29:48.73 -02:22:58.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:26.93 +16:50:53.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:31.15 -11:46:49.9 17.6mag P/2023 B1 (PANSTARRS)
09:19:25.09 -15:11:29.5 17.5mag C/2023 F3 (ATLAS)
21:30:57.63 +61:55:57.2 17.4mag C/2023 H5 (Lemmon)
19:31:10.10 -03:32:39.3 14.4mag C/2023 R1 (PANSTARRS)
21:40:53.91 +83:29:15.8 17.7mag C/2023 X2 (Lemmon)
06:13:59.96 +63:41:56.6 16.9mag C/2024 A1 (ATLAS)
04:25:46.30 +09:31:19.6 9.6mag C/2024 E1 (Wierzchos)
11:17:24.07 +03:59:24.1 18.0mag C/2024 G2 (ATLAS)
16:29:47.87 +03:11:24.5 17.4mag C/2024 G6 (ATLAS)
20:13:19.04 +10:16:15.7 14.8mag C/2024 J3 (ATLAS)
03:09:43.03 -25:32:23.0 16.4mag C/2024 T5 (ATLAS)
05:01:36.31 +50:36:53.6 17.6mag C/2025 J1 (Borisov)
14:54:33.60 +26:02:41.8 14.5mag C/2025 L1 (ATLAS)
02:56:48.99 -23:24:56.2 17.7mag C/2025 Q3 (ATLAS)
22:38:00.43 +19:26:43.1 11.6mag C/2025 R3 (PANSTARRS)
13:02:31.22 +01:44:36.7 17.6mag C/2025 Y1 (ATLAS)
01:50:50.32 -02:11:26.6 12.3mag C/2026 A1 (MAPS)
23:00:12.70 +32:52:23.7 13.9mag C/2026 B2 (Sun-Gao)
18:04:41.86 -10:37:46.8 12.9mag 10P/Tempel
15:22:38.97 +04:47:02.2 12.3mag 24P/Schaumasse
11:09:21.78 -02:13:53.7 15.6mag 29P/Schwassmann-Wachmann
17:49:45.29 -10:23:30.6 17.5mag 40P/Vaisala
10:42:05.65 -05:54:19.3 16.5mag 43P/Wolf-Harrington
01:18:41.52 +14:04:39.4 17.0mag 47P/Ashbrook-Jackson
06:37:44.42 +41:03:51.7 17.1mag 63P/Wild
23:03:09.17 -13:53:57.3 15.7mag 65P/Gunn
03:13:38.63 +13:57:28.1 15.9mag 76P/West-Kohoutek-Ikemura
00:23:08.71 +04:20:10.9 14.6mag 78P/Gehrels
22:00:40.78 -15:01:36.1 14.5mag 88P/Howell
01:17:16.75 +15:08:04.9 15.2mag 93P/Lovas
04:20:35.01 +31:06:43.4 16.4mag 123P/West-Hartley
08:10:32.61 +47:21:46.6 16.2mag 124P/Mrkos
02:03:42.42 +12:07:07.5 16.4mag 128P/Shoemaker-Holt
02:09:38.95 +11:56:22.9 17.4mag 131P/Mueller
23:49:07.17 +05:42:04.3 12.2mag 141P/Machholz
23:59:23.35 -02:17:32.4 12.3mag 141P-A/Machholz
22:55:59.58 -05:17:11.9 15.3mag 141P-D/Machholz
00:08:13.34 -11:08:10.0 15.4mag 162P/SidingSpring
10:35:18.22 +31:55:56.2 17.6mag 164P/Christensen
06:00:55.82 +24:41:18.6 17.6mag 198P/ODAS
15:24:25.60 -02:29:13.2 17.1mag 210P/Christensen
20:35:43.34 -16:07:19.0 17.2mag 218P/LINEAR
17:05:32.02 -16:05:16.8 16.2mag 235P/LINEAR
04:53:54.44 +32:48:24.1 16.4mag 240P/NEAT
07:31:09.89 -07:30:44.7 17.5mag 242P/Spahr
15:47:57.89 +05:35:11.5 17.6mag 391P/Kowalski
07:28:46.41 +21:12:20.7 17.6mag 450P/LONEOS
05:08:57.24 +46:12:21.2 17.3mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 27 07:33 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 27 07:33 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 27 07:34 tocp_transients_list.txt