This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw
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,2461120.5841,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.0841 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:12:13.29 +73:46:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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!
TCP 2026 03 21.0841* 23 53 52.54 +65 48 48.8 11.2 U Cas 9 0
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,2461120.5841,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.0841 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:53:52.54 +65:48:48.8 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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!
TCP 2026 03 21.0841* 01 05 58.71 +67 30 39.3 11.4 U Cas 9 0
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,2461120.5841,11.39,0.05,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 20260321.0841 11.39CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:05:58.71 +67:30:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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!
TCP 2026 03 21.0841* 01 02 07.53 +70 59 53.4 11.5 U Cas 9 0
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,2461120.5841,11.46,0.05,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 20260321.0841 11.46CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:02:07.53 +70:59:53.4 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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!
TCP 2026 03 21.0841* 01 03 22.67 +66 03 00.3 11.5 U Cas 9 0
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,2461120.5841,11.48,0.05,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 20260321.0841 11.48CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:03:22.67 +66:03:00.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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
HP Cep,2461120.5841,11.72,0.05,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
HP Cep 20260321.0841 11.72CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:49.11 +65:44:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 13.84 23:12:40.18 +65:30:05.6
112.92449 4.56709 galactic Cep Second-epoch detections are separated by 8.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:12:40.18 +65:30:05.6 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.170 (K)
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
target,2461120.5841,13.84,0.05,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 20260321.0841 13.84CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:40.18 +65:30:05.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 13.59 00:04:41.65 +72:19:15.4
119.35339 9.77474 galactic Cep Second-epoch detections are separated by 8.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:04:41.65 +72:19:15.4 (user input) | T | P | (position from user input) J-Ks=0.305+/- (F)
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
target,2461120.5841,13.59,0.05,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 20260321.0841 13.59CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:04:41.65 +72:19:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.38,0.05,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 20260321.0841 13.38CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:06:56.07 +72:42:53.5 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 9.52 22:59:56.94 +65:39:41.3
111.77617 5.23385 galactic Cep Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2211865246426788480 | 22:59:55.93 +65:39:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211865246426788480,2461120.5841,9.52,0.05,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 2211865246426788480 20260321.0841 9.52CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:56.94 +65:39:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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 J225950.96+662119.3,2461120.5841,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J225950.96+662119.3 20260321.0841 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:51.28 +66:21:28.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 11.73 23:00:35.81 +65:22:52.7
111.72024 4.95119 galactic Cep Second-epoch detections are separated by 4.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2211843256194352256 | 23:00:36.00 +65:22:43.6 (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 2211843256194352256,2461120.5841,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211843256194352256 20260321.0841 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:35.81 +65:22:52.7 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 11.85 23:01:32.89 +65:31:27.8
111.86996 5.04057 galactic Cep Second-epoch detections are separated by 5.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2211870915780376448 | 23:01:33.11 +65:31:17.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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
Large-amplitude variable Gaia DR2 2211870915780376448,2461120.5841,11.85,0.05,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
Large-amplitude variable Gaia DR2 2211870915780376448 20260321.0841 11.85CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:01:32.89 +65:31:27.8 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 11.97 23:00:21.80 +65:30:03.4
111.74803 5.07009 galactic Cep Second-epoch detections are separated by 6.2" and 4.7 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 2211847924818923520 | 23:00:22.79 +65:29:54.8 (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 2211847924818923520,2461120.5841,11.97,0.05,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
Gaia DR3 2211847924818923520 20260321.0841 11.97CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:21.80 +65:30:03.4 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 12.07 23:00:34.23 +65:14:52.9
111.66216 4.83110 galactic Cep Second-epoch detections are separated by 5.4" and 4.9 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 | Gaia DR3 2208839184269628416 | 23:00:34.69 +65:14:43.5 (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 2208839184269628416,2461120.5841,12.07,0.05,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 2208839184269628416 20260321.0841 12.07CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:34.23 +65:14:52.9 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 12.36 22:59:17.17 +66:24:09.9
112.02699 5.93507 galactic Cep Second-epoch detections are separated by 8.3" and 4.7 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 2212166684411521664 | 22:59:17.67 +66:23:58.3 (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 2212166684411521664,2461120.5841,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212166684411521664 20260321.0841 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:17.17 +66:24:09.9 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 12.36 23:02:03.60 +65:09:26.6
111.76736 4.68408 galactic Cep Second-epoch detections are separated by 8.5" and 4.9 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 | Gaia DR3 2208845742680876032 | 23:02:04.33 +65:09:18.4 (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 2208845742680876032,2461120.5841,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208845742680876032 20260321.0841 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:02:03.60 +65:09:26.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,12.87,0.05,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 20260321.0841 12.87CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:01:01.04 +73:33:09.5 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 13.00 23:00:46.53 +65:15:42.0
111.68743 4.83461 galactic Cep Second-epoch detections are separated by 6.7" and 4.9 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 | Gaia DR3 2208839287348844160 | 23:00:47.39 +65:15:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2208839287348844160,2461120.5841,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2208839287348844160 20260321.0841 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:46.53 +65:15:42.0 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 13.06 23:01:32.21 +65:23:38.6
111.81496 4.92231 galactic Cep Second-epoch detections are separated by 8.5" and 5.0 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 2211866105420386816 | 23:01:32.79 +65:23:23.3 (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 2211866105420386816,2461120.5841,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2211866105420386816 20260321.0841 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:01:32.21 +65:23:38.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.28,0.05,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 20260321.0841 13.28CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:56:57.15 +72:46:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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
NSVS J2309464+651720,2461120.5841,13.50,0.05,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
NSVS J2309464+651720 20260321.0841 13.50CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:45.33 +65:17:37.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.55,0.05,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 20260321.0841 13.55CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:02:28.27 +70:12:39.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.46,0.05,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 20260321.0841 13.46CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:39.89 +65:20:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.85,0.05,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
target 20260321.0841 13.85CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:04:04.55 +65:34:06.9 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.93,0.05,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 20260321.0841 13.93CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:46:00.20 +72:21:35.8 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,13.88,0.05,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 20260321.0841 13.88CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:59:44.27 +72:31:42.2 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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,2461120.5841,14.28,0.05,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 20260321.0841 14.28CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:53:28.80 +72:42:01.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 12.57 23:02:01.24 +66:27:07.5
112.29757 5.86624 galactic Cep Second-epoch detections are separated by 8.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2212161186853705600 | 23:02:01.95 +66:26:58.6 (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 2212161186853705600,2461120.5841,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212161186853705600 20260321.0841 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:02:01.24 +66:27:07.5 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1301,2461120.5841,12.85,0.05,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
Mis V1301 20260321.0841 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:02.84 +67:50:18.8 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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 J230015.68+663615.8,2461120.5841,12.21,0.05,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
ASASSN-V J230015.68+663615.8 20260321.0841 12.21CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:15.21 +66:36:26.6 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.0841 2461120.5841 12.53 23:12:44.17 +66:10:03.2
113.18016 5.18248 galactic Cep Second-epoch detections are separated by 7.6" and 4.9 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 | Gaia DR3 2209011223482722176 | 23:12:45.01 +66:09:56.9 (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 2209011223482722176,2461120.5841,12.53,0.05,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 2209011223482722176 20260321.0841 12.53CV 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:44.17 +66:10:03.2 ;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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20_00sec_-15_00C_LIGHT_0010_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: 2461032.68385993 23.12.2025 04:24:35.498 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
First image: 2461032.68385993 23.12.2025 04:24:35.498 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Last image: 2461120.58436742 21.03.2026 02:01:19.345 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16395
Objects passed selection criteria: 16330
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: 12897.5
Average stars matched: 12481.5 (96.7746 %)
Memory usage VmPeak: 121728 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 21:04:44 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: 2461032.68385993 23.12.2025 04:24:35.498 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
First image: 2461032.68385993 23.12.2025 04:24:35.498 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Last image: 2461120.58436742 21.03.2026 02:01:19.345 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 275
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 42 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): 107723
Objects passed selection criteria: 107550
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 90151.5
Average stars matched: 86356.8 (95.7907 %)
Memory usage VmPeak: 1886648 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 21:16:44 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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: 2461120.58380493
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits'
wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits'
wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits'
wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits exists and is non-empty
Saving wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits to local_wcs_cache/
'wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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 00:00:09.225 +69:59:33.46
Second-epoch image center 23:58:40.829 +70:00:19.55
Angular distance between the image centers 0.13 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 00:00:09.225 +69:59:33.46
Second-epoch image center 23:58:38.155 +69:59:53.48
Angular distance between the image centers 0.13 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 23:58:40.829 +70:00:19.55
Second-epoch second image center 23:58:38.155 +69:59:53.48
Angular distance between the image centers 0.00818 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits &> /tmp/tmp.InAyOaLuUk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits &> /tmp/tmp.6NbR9e6xmQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits &> /tmp/tmp.kJoL4QfIm6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.6BF6h35JWI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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 9732 out of 19885 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.943366
a=0.000000 b=1.000000 c=22.943366
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
2.2 pix Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
2.5 pix fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
2.5 pix fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Limiting magnitude estimates:
15.3 mag. Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
15.3 mag. Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
14.5 mag. fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
14.5 mag. fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.InAyOaLuUk (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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1699, passed=19885
Got 19885 stars (including 18167 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 19885 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits -region wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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.6NbR9e6xmQ (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/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1660, passed=19864
Got 19864 stars (including 18173 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 19864 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits -region wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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.kJoL4QfIm6 (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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=797, passed=10556
Got 10556 stars (including 9746 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 10556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.5'
Seting catalog search parameters based on the expected field of view 922.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012813 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010250 (36.9 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 258 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: 9.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.20"
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 325 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.61"
Estimated accuracy of the plate solution: 7.34"
Excluding outliers - 282 stars left (next iteration limit 223)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.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.6BF6h35JWI (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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=833, passed=10965
Got 10965 stars (including 10121 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 10965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 261 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: 9.96"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 334 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.40"
Estimated accuracy of the plate solution: 7.51"
Excluding outliers - 283 stars left (next iteration limit 229)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits'
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21417.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 5s
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Considering the candidate 21130_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21130_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 21224_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21224_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 21270_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21270_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 21295_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21295_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 21308_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 21308_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 21313_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21313_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 21334_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 21334_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 21417_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 21417_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 23s
Prepared the HTML report for the field Cep-03-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 ####
00:12:13.29 +73:46:09.1
23:53:52.54 +65:48:48.8
01:05:58.71 +67:30:39.3
01:02:07.53 +70:59:53.4
01:03:22.67 +66:03:00.3
22:59:49.11 +65:44:28.1
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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat to cache
SExtractor catalog cache: saved Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits exists and is non-empty
wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits exists and is non-empty
wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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 00:00:09.225 +69:59:33.46
Second-epoch image center 23:58:40.829 +70:00:19.55
Angular distance between the image centers 0.13 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 00:00:09.225 +69:59:33.46
Second-epoch image center 23:58:38.155 +69:59:53.48
Angular distance between the image centers 0.13 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 23:58:40.829 +70:00:19.55
Second-epoch second image center 23:58:38.155 +69:59:53.48
Angular distance between the image centers 0.00818 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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits &> /tmp/tmp.UKLRv7cPRK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits &> /tmp/tmp.yHHeNS9KGp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits &> /tmp/tmp.t8y2ywFpQR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.i3b1NOv1x9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
Found non-empty wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits and wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
The reference image (wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits) and catalog (wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat) found
'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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 9828 out of 129657 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808518
a=0.000000 b=1.000000 c=22.808518
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 183 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
2.2 pix Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
2.3 pix fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
2.3 pix fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Limiting magnitude estimates:
15.4 mag. Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
15.4 mag. Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
14.7 mag. fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
14.7 mag. fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UKLRv7cPRK (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/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=13735, passed=129640
Got 129640 stars (including 115675 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 129640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits -region wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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.yHHeNS9KGp (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/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits' -> 'wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Checking if the catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
WCS catalog name: wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=13645, passed=128922
Got 128922 stars (including 115067 good ones) from the SExtractor catalog wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 128922 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits -region wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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.t8y2ywFpQR (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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=5781, passed=72145
Got 72145 stars (including 66245 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 72145 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.5'
Seting catalog search parameters based on the expected field of view 922.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012813 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010250 (36.9 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 244 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: 9.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.20"
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 302 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.07"
Estimated accuracy of the plate solution: 7.64"
Excluding outliers - 262 stars left (next iteration limit 205)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.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.i3b1NOv1x9 (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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=6198, passed=75232
Got 75232 stars (including 68928 good ones) from the SExtractor catalog wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 75232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 922.6'
Seting catalog search parameters based on the expected field of view 922.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012814 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010251 (36.9 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 246 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: 9.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.06"
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 303 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.02"
Estimated accuracy of the plate solution: 6.53"
Excluding outliers - 254 stars left (next iteration limit 201)
The image catalog is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_Cep-03-Q2b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits
Saving fully-calibrated image wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_Cep-03-Q2b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-00-30_20.00sec_-15.00C_LIGHT_0010.fits
Saving fully-calibrated image wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.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_2026-03-20_CI_Cep-03-Q2b1x1_210227_TTUQ2b1x1_14844_uTQFN1vw/wcs_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011.fits
Preparing the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out149315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96432.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 48s
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: 17s
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Considering the candidate 149066_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149066_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 149075_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149075_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (38.0") between the two second-epoch detections
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Considering the candidate 149078_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149078_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 149098_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149098_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 149101_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149101_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 149102_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149102_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 149103_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149103_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 149109_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149109_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 149110_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149110_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (38.6") between the two second-epoch detections
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Considering the candidate 149113_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149113_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 149114_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149114_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149116_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149116_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 149117_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149117_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 149127_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149127_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 149128_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149128_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149129_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149129_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 149131_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149131_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 149132_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149132_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 149133_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149133_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 149135_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149135_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 149138_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149138_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 149139_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149139_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 149143_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149143_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 149150_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149150_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 149151_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149151_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149156_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149156_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 149158_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149158_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 149164_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149164_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 149165_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149165_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 149167_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149167_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 149169_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149169_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 149172_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149172_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 149173_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149173_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 149174_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149174_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 149176_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149176_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 149178_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149178_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (35.9") between the two second-epoch detections
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Considering the candidate 149262_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149262_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149315_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149315_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
**** FOUND 23:05:03.11 +65:14:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.02, MAG_FAINT_SEARCH_LIMIT=11.00)GAIADR2_OUTPUT=# 1.648 2208849286033178240 346.26186653377 +65.24110377195 9.4770 8.5440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149452_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149452_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149467_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149467_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
**** FOUND 23:02:18.24 +65:10:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 4.554 2208845953138151936 345.57701521976 +65.17905882239 10.4913 9.6491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149527_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149527_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 149528_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149528_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 149539_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149539_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 149724_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149724_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149782_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149782_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149887_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149887_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149935_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 149935_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 149937_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 149937_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 150182_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 150182_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 150188_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 150188_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 150240_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150240_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 150282_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150282_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
**** FOUND 23:18:15.70 +68:07:24.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 150290_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150290_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 150313_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150313_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 150329_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150329_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 150355_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150355_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 150372_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150372_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 150432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 150444_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150444_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 150477_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150477_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 150625_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 150625_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 150632_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150632_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 150704_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150704_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 150708_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150708_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 150731_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150731_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 150744_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150744_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 150777_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150777_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 150861_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150861_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 150872_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150872_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 150893_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 150893_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 150923_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 150923_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 150996_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 150996_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 151021_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151021_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 151077_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151077_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 151095_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151095_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 151130_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151130_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 151138_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151138_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 151150_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151150_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 151157_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151157_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 151211_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151211_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 151212_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151212_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 151255_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151255_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 151272_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151272_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 151276_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151276_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 151282_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151282_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 151291_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151291_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 151314_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151314_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 151324_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 151324_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 151338_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151338_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 151340_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151340_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 151391_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151391_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 151397_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151397_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 151459_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151459_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 151483_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151483_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 151488_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151488_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 151493_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151493_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 151529_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151529_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 151541_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151541_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 151577_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151577_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 151600_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151600_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 151636_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151636_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 151641_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151641_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 151659_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151659_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 151681_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151681_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 151691_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151691_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (41.5") between the two second-epoch detections
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Considering the candidate 151720_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151720_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 151727_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151727_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 151752_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151752_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 151754_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151754_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 151772_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 151772_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 151792_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 151792_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 151800_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151800_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 151828_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151828_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 151850_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 151850_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 151897_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151897_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 151898_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151898_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 151934_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151934_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
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Considering the candidate 151942_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151942_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 151944_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151944_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (48.1") between the two second-epoch detections
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Considering the candidate 151952_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151952_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 151977_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151977_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 151978_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 151978_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 152015_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152015_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (48.1") between the two second-epoch detections
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Considering the candidate 152044_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152044_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 152068_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152068_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 152087_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152087_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 152093_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152093_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 152105_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152105_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 152126_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152126_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 152154_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152154_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 152209_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152209_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 152211_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152211_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 152240_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152240_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 152242_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152242_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (36.1") between the two second-epoch detections
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Considering the candidate 152263_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152263_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 152275_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 152275_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 152286_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152286_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 152291_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152291_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 152303_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152303_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 152330_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152330_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 152337_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152337_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 152416_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152416_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 152426_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 152426_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 152432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 152461_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152461_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 152493_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152493_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 152556_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152556_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 152575_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152575_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (30.0") between the two second-epoch detections
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Considering the candidate 152591_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152591_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 152598_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152598_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 152664_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152664_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 152676_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 152676_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 152717_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152717_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (35.8") between the two second-epoch detections
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Considering the candidate 152732_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152732_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 152760_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152760_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 152764_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152764_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 152872_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152872_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 152893_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 152893_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 153035_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153035_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 153038_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153038_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 153057_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153057_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (30.0") between the two second-epoch detections
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Considering the candidate 153081_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 153081_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
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Considering the candidate 153114_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153114_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 153278_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153278_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 153283_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153283_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 153316_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 153316_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 140932_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 140932_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
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Considering the candidate 15288_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 15288_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 25686_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 25686_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 148413_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 148413_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 101518_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 101518_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34593_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 34593_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118483_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 118483_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83874_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 83874_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103584_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 103584_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141585_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 141585_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141511_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 141511_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
Preparing report for the candidate 96432_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72846_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 72846_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71073_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 71073_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52310_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 52310_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129396_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 129396_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36182_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011
The candidate 36182_fd_Cep-03-Q2b1x1_2026-03-20_21-01-19_20.00sec_-15.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 70s
Prepared the HTML report for the field Cep-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:12:13.29 +73:46:09.1
23:53:52.54 +65:48:48.8
01:05:58.71 +67:30:39.3
01:02:07.53 +70:59:53.4
01:03:22.67 +66:03:00.3
22:59:49.11 +65:44:28.1
23:02:01.24 +66:27:07.5
23:00:15.21 +66:36:26.6
23:08:02.84 +67:50:18.8
23:12:40.18 +65:30:05.6
00:04:41.65 +72:19:15.4
00:06:56.07 +72:42:53.5
22:59:56.94 +65:39:41.3
22:59:51.28 +66:21:28.6
23:00:35.81 +65:22:52.7
23:01:32.89 +65:31:27.8
23:00:21.80 +65:30:03.4
23:00:34.23 +65:14:52.9
22:59:17.17 +66:24:09.9
23:02:03.60 +65:09:26.6
00:01:01.04 +73:33:09.5
23:00:46.53 +65:15:42.0
23:01:32.21 +65:23:38.6
23:56:57.15 +72:46:35.3
23:09:45.33 +65:17:37.6
23:02:28.27 +70:12:39.1
23:00:39.89 +65:20:58.6
23:04:04.55 +65:34:06.9
23:46:00.20 +72:21:35.8
23:59:44.27 +72:31:42.2
23:53:28.80 +72:42:01.6
23:12:44.17 +66:10:03.2
########### Completed Cep-03-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 ####
00:12:13.29 +73:46:09.1
23:53:52.54 +65:48:48.8
01:05:58.71 +67:30:39.3
01:02:07.53 +70:59:53.4
01:03:22.67 +66:03:00.3
22:59:49.11 +65:44:28.1
23:12:40.18 +65:30:05.6
00:04:41.65 +72:19:15.4
00:06:56.07 +72:42:53.5
22:59:56.94 +65:39:41.3
22:59:51.28 +66:21:28.6
23:00:35.81 +65:22:52.7
23:01:32.89 +65:31:27.8
23:00:21.80 +65:30:03.4
23:00:34.23 +65:14:52.9
22:59:17.17 +66:24:09.9
23:02:03.60 +65:09:26.6
00:01:01.04 +73:33:09.5
23:00:46.53 +65:15:42.0
23:01:32.21 +65:23:38.6
23:56:57.15 +72:46:35.3
23:09:45.33 +65:17:37.6
23:02:28.27 +70:12:39.1
23:00:39.89 +65:20:58.6
23:04:04.55 +65:34:06.9
23:46:00.20 +72:21:35.8
23:59:44.27 +72:31:42.2
23:53:28.80 +72:42:01.6
23:02:01.24 +66:27:07.5
23:08:02.84 +67:50:18.8
23:00:15.21 +66:36:26.6
23:12:44.17 +66:10:03.2
###################################################################################
00:12:13.29 +73:46:09.1 -- not an asteroid (will add it to exclusion list)
23:53:52.54 +65:48:48.8 -- not an asteroid (will add it to exclusion list)
01:05:58.71 +67:30:39.3 -- not an asteroid (will add it to exclusion list)
01:02:07.53 +70:59:53.4 -- not an asteroid (will add it to exclusion list)
01:03:22.67 +66:03:00.3 -- not an asteroid (will add it to exclusion list)
22:59:49.11 +65:44:28.1 -- not an asteroid (will add it to exclusion list)
23:12:40.18 +65:30:05.6 -- not an asteroid (will add it to exclusion list)
00:04:41.65 +72:19:15.4 -- not an asteroid (will add it to exclusion list)
00:06:56.07 +72:42:53.5 -- not an asteroid (will add it to exclusion list)
22:59:56.94 +65:39:41.3 -- not an asteroid (will add it to exclusion list)
22:59:51.28 +66:21:28.6 -- not an asteroid (will add it to exclusion list)
23:00:35.81 +65:22:52.7 -- not an asteroid (will add it to exclusion list)
23:01:32.89 +65:31:27.8 -- not an asteroid (will add it to exclusion list)
23:00:21.80 +65:30:03.4 -- not an asteroid (will add it to exclusion list)
23:00:34.23 +65:14:52.9 -- not an asteroid (will add it to exclusion list)
22:59:17.17 +66:24:09.9 -- not an asteroid (will add it to exclusion list)
23:02:03.60 +65:09:26.6 -- not an asteroid (will add it to exclusion list)
00:01:01.04 +73:33:09.5 -- not an asteroid (will add it to exclusion list)
23:00:46.53 +65:15:42.0 -- not an asteroid (will add it to exclusion list)
23:01:32.21 +65:23:38.6 -- not an asteroid (will add it to exclusion list)
23:56:57.15 +72:46:35.3 -- not an asteroid (will add it to exclusion list)
23:09:45.33 +65:17:37.6 -- not an asteroid (will add it to exclusion list)
23:02:28.27 +70:12:39.1 -- not an asteroid (will add it to exclusion list)
23:00:39.89 +65:20:58.6 -- not an asteroid (will add it to exclusion list)
23:04:04.55 +65:34:06.9 -- not an asteroid (will add it to exclusion list)
23:46:00.20 +72:21:35.8 -- not an asteroid (will add it to exclusion list)
23:59:44.27 +72:31:42.2 -- not an asteroid (will add it to exclusion list)
23:53:28.80 +72:42:01.6 -- not an asteroid (will add it to exclusion list)
23:02:01.24 +66:27:07.5 -- not an asteroid (will add it to exclusion list)
23:08:02.84 +67:50:18.8 -- not an asteroid (will add it to exclusion list)
23:00:15.21 +66:36:26.6 -- not an asteroid (will add it to exclusion list)
23:12:44.17 +66:10:03.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:01.04 +73:33:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:41.65 +72:19:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:56.07 +72:42:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:13.29 +73:46:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:07.53 +70:59:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:22.67 +66:03:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:58.71 +67:30:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:17.17 +66:24:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:49.11 +65:44:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:51.28 +66:21:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:59:56.94 +65:39:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:15.21 +66:36:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:21.80 +65:30:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:34.23 +65:14:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:35.81 +65:22:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:39.89 +65:20:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:46.53 +65:15:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:32.21 +65:23:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:01:32.89 +65:31:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:01.24 +66:27:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:03.60 +65:09:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:02:28.27 +70:12:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:04:04.55 +65:34:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:02.84 +67:50:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:45.33 +65:17:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:40.18 +65:30:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:44.17 +66:10:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:00.20 +72:21:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:28.80 +72:42:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:52.54 +65:48:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:57.15 +72:46:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:44.27 +72:31:42.2 -- 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)
00:01:01.04 +73:33:09.5 -- not a known variable star
00:04:41.65 +72:19:15.4 -- not a known variable star
00:06:56.07 +72:42:53.5 -- not a known variable star
00:12:13.29 +73:46:09.1 -- not a known variable star
01:02:07.53 +70:59:53.4 -- not a known variable star
01:03:22.67 +66:03:00.3 -- not a known variable star
01:05:58.71 +67:30:39.3 -- not a known variable star
22:59:17.17 +66:24:09.9 -- not a known variable star
22:59:49.11 +65:44:28.1 -- a known variable star
22:59:51.28 +66:21:28.6 -- a known variable star
22:59:56.94 +65:39:41.3 -- not a known variable star
23:00:15.21 +66:36:26.6 -- a known variable star
23:00:21.80 +65:30:03.4 -- not a known variable star
23:00:34.23 +65:14:52.9 -- not a known variable star
23:00:35.81 +65:22:52.7 -- not a known variable star
23:00:39.89 +65:20:58.6 -- not a known variable star
23:00:46.53 +65:15:42.0 -- not a known variable star
23:01:32.21 +65:23:38.6 -- not a known variable star
23:01:32.89 +65:31:27.8 -- not a known variable star
23:02:01.24 +66:27:07.5 -- not a known variable star
23:02:03.60 +65:09:26.6 -- not a known variable star
23:02:28.27 +70:12:39.1 -- not a known variable star
23:04:04.55 +65:34:06.9 -- not a known variable star
23:08:02.84 +67:50:18.8 -- a known variable star
23:09:45.33 +65:17:37.6 -- a known variable star
23:12:40.18 +65:30:05.6 -- not a known variable star
23:12:44.17 +66:10:03.2 -- not a known variable star
23:46:00.20 +72:21:35.8 -- not a known variable star
23:53:28.80 +72:42:01.6 -- not a known variable star
23:53:52.54 +65:48:48.8 -- not a known variable star
23:56:57.15 +72:46:35.3 -- not a known variable star
23:59:44.27 +72:31:42.2 -- not a known variable star
Found 27 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
32 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 ####
00:01:01.04 +73:33:09.5
00:04:41.65 +72:19:15.4
00:06:56.07 +72:42:53.5
00:12:13.29 +73:46:09.1
01:02:07.53 +70:59:53.4
01:03:22.67 +66:03:00.3
01:05:58.71 +67:30:39.3
22:59:17.17 +66:24:09.9
22:59:49.11 +65:44:28.1
22:59:51.28 +66:21:28.6
22:59:56.94 +65:39:41.3
23:00:15.21 +66:36:26.6
23:00:21.80 +65:30:03.4
23:00:34.23 +65:14:52.9
23:00:35.81 +65:22:52.7
23:00:39.89 +65:20:58.6
23:00:46.53 +65:15:42.0
23:01:32.21 +65:23:38.6
23:01:32.89 +65:31:27.8
23:02:01.24 +66:27:07.5
23:02:03.60 +65:09:26.6
23:02:28.27 +70:12:39.1
23:04:04.55 +65:34:06.9
23:08:02.84 +67:50:18.8
23:09:45.33 +65:17:37.6
23:12:40.18 +65:30:05.6
23:12:44.17 +66:10:03.2
23:46:00.20 +72:21:35.8
23:53:28.80 +72:42:01.6
23:53:52.54 +65:48:48.8
23:56:57.15 +72:46:35.3
23:59:44.27 +72:31:42.2
23:05:03.11 +65:14:27.9
23:02:18.24 +65:10:48.9
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461120.58380493 -observatory 500
22:37:43.78 -07:40:01.8 Mercury (1.0mag)
01:06:57.41 +06:11:28.4 Venus (-3.9mag)
23:03:24.75 -07:12:47.3 Mars (1.2mag)
07:04:46.46 +22:57:59.9 Jupiter (-2.3mag)
00:17:23.23 -00:25:55.7 Saturn (0.9mag)
03:42:56.89 +19:31:55.0 Uranus (5.8mag)
00:07:18.10 -00:37:57.7 Neptune (7.8mag)
20:32:00.78 -22:53:47.0 Pluto (14.5mag)
01:33:57.64 +14:00:39.6 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 361 Mar 20 21:04 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461120.58380493:
07:04:53.84 +22:57:44.7 Io (5.6mag)
07:04:32.64 +22:58:26.2 Europa (5.7mag)
07:04:25.25 +22:58:37.2 Ganymede (5.2mag)
07:04:10.69 +22:59:01.2 Callisto (6.4mag)
07:08:47.77 +22:59:33.8 Himalia (15.2mag)
07:04:46.18 +22:58:02.9 Thebe (16.0mag)
07:08:22.72 +23:22:52.9 Elara (17.2mag)
07:01:54.80 +23:51:38.2 Pasiphae (17.2mag)
07:13:33.83 +22:52:28.2 Carme (18.3mag)
00:17:17.60 -00:25:51.3 Titan (8.8mag)
00:17:28.13 -00:25:54.7 Rhea (10.1mag)
00:17:52.90 -00:23:53.3 Iapetus (11.5mag)
00:17:38.34 -00:26:01.1 Hyperion (14.8mag)
00:19:17.33 -00:14:39.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 20 21:04 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461120.58380493:
12:50:35.80 +08:45:59.9 JWST
16:03:52.67 +50:08:00.1 Chandra
07:37:55.63 -21:18:08.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 20 21:04 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461120.58380493 -observatory 500
18:35:29.17 -27:27:55.3 14.1mag P/2010 H2 (Vales)
04:51:11.93 -71:01:42.9 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:44.22 +31:17:54.8 17.0mag C/2017 K2 (PANSTARRS)
17:29:39.01 +07:24:54.1 17.6mag C/2021 G2 (ATLAS)
23:01:35.50 +28:26:14.6 16.9mag C/2022 E2 (ATLAS)
04:00:34.73 +25:17:47.7 15.7mag C/2022 N2 (PANSTARRS)
09:01:52.64 +31:27:09.2 16.0mag C/2022 QE78 (ATLAS)
08:30:11.02 -03:09:59.8 17.2mag C/2022 R6 (PANSTARRS)
18:56:29.96 +16:17:55.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:21.09 -11:50:41.8 17.6mag P/2023 B1 (PANSTARRS)
09:24:27.47 -16:18:47.6 17.4mag C/2023 F3 (ATLAS)
21:21:49.53 +61:41:56.9 17.4mag C/2023 H5 (Lemmon)
19:33:10.94 -03:31:14.5 14.5mag C/2023 R1 (PANSTARRS)
21:36:26.50 +82:51:44.3 17.7mag C/2023 X2 (Lemmon)
06:15:21.87 +63:47:06.3 16.8mag C/2024 A1 (ATLAS)
04:06:40.46 +05:16:00.6 9.1mag C/2024 E1 (Wierzchos)
11:22:34.13 +02:44:50.5 18.0mag C/2024 G2 (ATLAS)
16:32:14.96 +02:10:40.1 17.5mag C/2024 G6 (ATLAS)
20:10:06.22 +08:46:59.9 14.9mag C/2024 J3 (ATLAS)
03:04:45.88 -26:38:19.6 16.5mag C/2024 T5 (ATLAS)
04:57:34.96 +52:34:44.9 17.6mag C/2025 J1 (Borisov)
15:13:33.96 +17:34:47.2 14.4mag C/2025 L1 (ATLAS)
02:48:37.56 -22:35:20.7 17.6mag C/2025 Q3 (ATLAS)
22:32:57.82 +19:01:13.7 12.5mag C/2025 R3 (PANSTARRS)
13:05:02.21 +01:19:03.5 17.6mag C/2025 Y1 (ATLAS)
02:09:35.03 -06:18:44.2 14.1mag C/2026 A1 (MAPS)
22:39:11.83 +31:04:07.1 13.7mag C/2026 B2 (Sun-Gao)
17:52:14.42 -10:50:20.3 13.3mag 10P/Tempel
15:26:45.82 +05:07:58.6 11.8mag 24P/Schaumasse
11:11:57.72 -02:28:40.4 15.6mag 29P/Schwassmann-Wachmann
17:43:45.39 -10:38:32.8 17.3mag 40P/Vaisala
10:45:06.31 -06:33:28.7 16.4mag 43P/Wolf-Harrington
01:09:04.98 +12:56:17.2 17.0mag 47P/Ashbrook-Jackson
06:28:41.50 +42:19:58.1 17.1mag 63P/Wild
22:54:18.97 -14:43:52.5 15.7mag 65P/Gunn
02:58:39.09 +11:21:25.7 15.9mag 76P/West-Kohoutek-Ikemura
00:09:41.34 +03:03:54.8 14.6mag 78P/Gehrels
21:39:02.18 -16:43:18.7 14.5mag 88P/Howell
01:00:58.19 +13:15:04.9 15.2mag 93P/Lovas
04:10:43.22 +30:41:26.2 16.5mag 123P/West-Hartley
08:07:47.98 +50:13:46.3 16.2mag 124P/Mrkos
01:54:27.35 +11:21:50.6 16.4mag 128P/Shoemaker-Holt
01:57:33.34 +11:02:41.5 17.4mag 131P/Mueller
23:20:27.53 +03:07:54.2 13.0mag 141P/Machholz
23:30:34.21 -04:24:20.0 13.0mag 141P-A/Machholz
22:31:16.33 -06:57:19.5 16.1mag 141P-D/Machholz
23:50:38.06 -14:06:35.4 15.5mag 162P/SidingSpring
10:39:17.53 +32:02:08.1 17.5mag 164P/Christensen
05:49:51.96 +24:44:14.8 17.5mag 198P/ODAS
15:33:15.14 -03:21:45.3 16.9mag 210P/Christensen
20:12:09.22 -17:31:46.1 17.2mag 218P/LINEAR
16:59:22.15 -16:40:09.0 16.3mag 235P/LINEAR
04:41:35.69 +32:00:38.1 16.3mag 240P/NEAT
07:29:53.49 -08:21:44.2 17.5mag 242P/Spahr
15:48:34.48 +05:06:37.1 17.7mag 391P/Kowalski
07:27:59.87 +21:06:32.1 17.5mag 450P/LONEOS
05:01:03.24 +46:36:42.6 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 20 21:04 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
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
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
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
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 20 21:04 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
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
-rw-r--r-- 1 apache apache 187K Mar 20 21:04 tocp_transients_list.txt