This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z
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,2461120.9056,13.73,0.05,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
target 20260321.4056 13.73CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:53:59.93 +63:47:43.2 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RT Cep,2461120.9056,13.53,0.05,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
RT Cep 20260321.4056 13.53CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:52.07 +64:36:02.5 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2240204+601216,2461120.9056,13.31,0.05,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 J2240204+601216 20260321.4056 13.31CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:19.25 +60:12:09.9 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J214839.36+594748.5,2461120.9056,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J214839.36+594748.5 20260321.4056 13.11CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:36.99 +59:47:41.1 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4056 2461120.9056 13.21 21:46:56.19 +64:35:52.7
104.71385 8.47033 galactic Cep Second-epoch detections are separated by 3.3" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | RT Cep | 21:46:52.64 +64:36:08.6 (Gaia DR3) | M (local) | 627.000000000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RT Cep,2461120.9056,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RT Cep 20260321.4056 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:56.19 +64:35:52.7 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J231259.00+642455.0,2461120.9056,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231259.00+642455.0 20260321.4056 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:57.93 +64:24:50.3 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4056 2461120.9056 13.70 21:44:48.54 +63:16:34.0
103.66583 7.61881 galactic Cep Second-epoch detections are separated by 0.5" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2216648426945292672 | 21:44:44.28 +63:16:06.6 (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 2216648426945292672,2461120.9056,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2216648426945292672 20260321.4056 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:48.54 +63:16:34.0 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4056 2461120.9056 13.72 21:28:07.50 +61:16:34.7
100.86115 7.45273 galactic Cep Second-epoch detections are separated by 1.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2192092587085556352 | 21:28:04.56 +61:16:19.2 (Gaia DR3) | VAR (local) | F (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2192092587085556352,2461120.9056,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2192092587085556352 20260321.4056 13.72CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:07.50 +61:16:34.7 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.9056,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.4056 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:36.89 +62:44:26.9 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2300355+631632,2461120.9056,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2300355+631632 20260321.4056 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:00:34.03 +63:16:23.0 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.4056 2461120.9056 14.14 22:04:50.28 +58:37:00.8
102.66437 2.46236 galactic Cep Second-epoch detections are separated by 5.0" and 0.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.2261+58.6224 | 22:04:50.28 +58:37:00.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.160+/-0.196 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.2261+58.6224,2461120.9056,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.2261+58.6224 20260321.4056 14.14CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:04:50.28 +58:37:00.8 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2224004+585003,2461120.9056,12.86,0.05,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 J2224004+585003 20260321.4056 12.86CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:23:58.58 +58:50:00.1 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1470590,2461120.9056,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1470590 20260321.4056 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:41.26 +64:39:59.6 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3503666,2461120.9056,12.01,0.05,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 3503666 20260321.4056 12.01CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:30:42.45 +63:56:59.3 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0894 Cep,2461120.9056,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0894 Cep 20260321.4056 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:36:30.59 +63:25:52.1 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J224312.75+592153.4,2461120.9056,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J224312.75+592153.4 20260321.4056 13.41CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:43:12.58 +59:21:53.5 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J224443.10+651132.1,2461120.9056,13.14,0.05,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 J224443.10+651132.1 20260321.4056 13.14CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:44:42.79 +65:11:27.0 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J223720.72+601850.1,2461120.9056,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J223720.72+601850.1 20260321.4056 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:37:20.55 +60:18:47.8 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2014636465544831744,2461120.9056,11.38,0.05,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
Gaia DR3 2014636465544831744 20260321.4056 11.38CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:54:20.40 +60:48:40.6 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J221122.87+592142.0,2461120.9056,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221122.87+592142.0 20260321.4056 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:22.54 +59:21:40.2 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2234553+594348,2461120.9056,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2234553+594348 20260321.4056 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:34:54.66 +59:43:44.3 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J224146.46+614241.8,2461120.9056,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J224146.46+614241.8 20260321.4056 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:41:46.35 +61:42:39.2 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0519 Cep,2461120.9056,13.49,0.05,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
V0519 Cep 20260321.4056 13.49CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:22:29.98 +64:09:19.3 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J221358.36+574813.3,2461120.9056,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221358.36+574813.3 20260321.4056 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:58.30 +57:48:10.9 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3511242,2461120.9056,12.46,0.05,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
NSVS 3511242 20260321.4056 12.46CV 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:27.34 +60:53:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1228 Cep,2461120.9056,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1228 Cep 20260321.4056 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:08.37 +62:10:11.8 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2307315+651201,2461120.9056,13.80,0.05,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 J2307315+651201 20260321.4056 13.80CV 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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:30.25 +65:11:55.2 ;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-06-Q2b1x1_2025-12-22_21-01-41_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20_00sec_-15_00C_LIGHT_0422_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
First image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Last image: 2461120.90585336 21.03.2026 09:44:15.730 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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): 24023
Objects passed selection criteria: 23957
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 19180.5
Average stars matched: 18154 (94.6482 %)
Memory usage VmPeak: 127156 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 Sat Mar 21 04:46:20 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: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
First image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Last image: 2461120.90585336 21.03.2026 09:44:15.730 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 310
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 50 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): 168341
Objects passed selection criteria: 167895
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 128138
Average stars matched: 120309 (93.8904 %)
Memory usage VmPeak: 1923864 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 Sat Mar 21 04:48:56 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
SExtractor catalog cache: saved Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat to cache
SExtractor catalog cache: saved Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461120.90533404
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits exists and is non-empty
Saving wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits to local_wcs_cache/
'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits exists and is non-empty
Saving wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits to local_wcs_cache/
'wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits'
wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits exists and is non-empty
Saving wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits to local_wcs_cache/
'wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits' -> 'local_wcs_cache/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits'
wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:52.388 +62:00:21.94
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:53.188 +62:00:18.34
Angular distance between the image centers 0.04 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 22:16:52.388 +62:00:21.94
Second-epoch second image center 22:16:53.188 +62:00:18.34
Angular distance between the image centers 0.00186 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits &> /tmp/tmp.Zpwgb2FCQQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits &> /tmp/tmp.YXXZKqx5C3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits &> /tmp/tmp.3SnoXmCYLk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.ryw3VT131I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
Found non-empty wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
The reference image (wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits) and catalog (wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat) found
'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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 13829 out of 26505 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.945131
a=0.000000 b=1.000000 c=22.945131
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
2.1 pix Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
3.0 pix fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
3.0 pix fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Limiting magnitude estimates:
15.2 mag. Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
15.2 mag. Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
14.6 mag. fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
14.6 mag. fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.9 (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.Zpwgb2FCQQ (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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> 'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Checking if the catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS catalog name: wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3069, passed=26505
Got 26505 stars (including 23407 good ones) from the SExtractor catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 26505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 974 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits -region wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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.YXXZKqx5C3 (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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits' -> 'wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Checking if the catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS catalog name: wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3047, passed=26453
Got 26453 stars (including 23360 good ones) from the SExtractor catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 26453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 974 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits -region wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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.3SnoXmCYLk (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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Checking if the catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS catalog name: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1185, passed=18443
Got 18443 stars (including 17249 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 18443 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.82"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits -region wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ryw3VT131I (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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1196, passed=18502
Got 18502 stars (including 17295 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 18502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
Saving fully-calibrated image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits'
Saving fully-calibrated image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits'
Saving fully-calibrated image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits'
Preparing the HTML report for the field Cep-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33927.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 32276_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 32276_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:49:16.39 +58:35:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32912_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 32912_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:53:46.16 +60:32:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32952_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 32952_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:04:29.00 +64:45:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33265_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33265_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:59:48.40 +65:44:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33319_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33319_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:30:42.49 +63:56:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.258 2205522438725652864 337.67754550799 +63.95068309778 10.0592 8.5106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33518_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33518_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:31:57.02 +60:13:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.700 2200926617565768832 337.98809620467 +60.23098116328 10.6973 9.2483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:40:59.62 +58:44:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33608_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33608_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:19:14.06 +61:22:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.118 2204656367161337856 334.80863949761 +61.37767096452 10.7536 9.3653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33730_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33730_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:15:34.25 +62:22:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.185 2204958801579547392 333.89295860583 +62.37415119727 11.9863 11.5383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33901_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33901_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:26:26.51 +63:06:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.372 2205391729982249728 336.61070280069 +63.11161479106 12.4661 11.8271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33923_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33923_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:55:39.43 +62:50:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.065 2207285230736719744 343.91414081351 +62.85012512249 12.3054 11.4629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33927_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 33927_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:51:19.05 +65:01:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.727 2211514948894013824 342.83001320667 +65.01973555909 11.8461 10.8552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31001_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 31001_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:37:36.12 +61:16:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31054_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 31054_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:34:54.71 +59:43:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.600 2200656927976323328 338.72925763608 +59.72924855423 10.4369 8.8562 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19289_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 19289_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:26:40.31 +58:31:35.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cep-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
SExtractor catalog cache: saved Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat to cache
SExtractor catalog cache: saved Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Creating symlink local_wcs_cache/wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits exists and is non-empty
wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits exists and is non-empty
wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits exists and is non-empty
wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:52.388 +62:00:21.94
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:53.188 +62:00:18.34
Angular distance between the image centers 0.04 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 22:16:52.388 +62:00:21.94
Second-epoch second image center 22:16:53.188 +62:00:18.34
Angular distance between the image centers 0.00186 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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits &> /tmp/tmp.6aRE8v88Bp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits &> /tmp/tmp.l1lJs2UjdV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits &> /tmp/tmp.JQBwjOB7ef
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.uO0JjUCOkF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
Found non-empty wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
The reference image (wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits) and catalog (wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat) found
'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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 14307 out of 188195 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803185
a=0.000000 b=1.000000 c=22.803185
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 238 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
1.9 pix Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
2.9 pix fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
2.8 pix fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Limiting magnitude estimates:
15.4 mag. Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
15.4 mag. Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
14.6 mag. fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
14.6 mag. fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.6aRE8v88Bp (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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> 'wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Checking if the catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS catalog name: wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=27430, passed=188152
Got 188152 stars (including 160411 good ones) from the SExtractor catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 188152 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits -region wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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.l1lJs2UjdV (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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits' -> 'wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Checking if the catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
WCS catalog name: wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=27390, passed=188660
Got 188660 stars (including 160954 good ones) from the SExtractor catalog wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 188660 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 974 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits -region wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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.JQBwjOB7ef (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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Checking if the catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
WCS catalog name: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=10228, passed=95926
Got 95926 stars (including 85621 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 95926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits -region wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uO0JjUCOkF (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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=10535, passed=98790
Got 98790 stars (including 88159 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 98790 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Saving fully-calibrated image wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.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_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits
Saving fully-calibrated image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-43-30_20.00sec_-15.00C_LIGHT_0422.fits
Saving fully-calibrated image wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Cep-06-Q2b1x1_044454_TTUQ2b1x1_21122_lLITjs2z/wcs_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423.fits
Preparing the HTML report for the field Cep-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out199540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out220073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out220597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out221370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out221553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out222812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out223553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out226830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out104540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out221953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out223397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92206.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 13s
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Considering the candidate 213519_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213519_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:27:19.32 +64:45:48.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 213526_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213526_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:46:07.16 +62:11:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213527_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213527_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 213532_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213532_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:48:31.30 +58:52:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.922 2202597016251111168 327.13031792057 +58.87094797790 13.8796 13.2256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213536_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213536_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 213541_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213541_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:00:24.59 +60:11:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213551_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 213551_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 213559_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 213559_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 213560_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213560_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:20:31.98 +61:08:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213562_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 213562_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 213566_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213566_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 213568_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213568_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:34:03.78 +61:49:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213571_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 213571_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 213574_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 213574_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 214710_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 214710_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:12:41.58 +63:56:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215057_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 215057_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:45:11.66 +61:08:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 1.647 2203889320366911872 326.29900616816 +61.14199270504 11.5801 11.1547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215482_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 215482_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:59:48.41 +65:44:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215644_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 215644_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 215964_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 215964_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:02:13.32 +58:01:21.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 216379_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216379_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 216482_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216482_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 216692_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216692_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:01:56.31 +57:58:59.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 216829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 216986_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216986_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 216999_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 216999_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217217_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217217_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217238_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217238_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:03:55.78 +64:35:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.129 2218143835781543168 330.98298461668 +64.59361396193 12.7657 12.3503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 217285_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217285_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217491_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217491_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217544_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217544_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217545_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217545_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217567_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217567_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217710_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217710_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217773_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217773_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217882_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217882_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 217887_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217887_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:54:08.46 +62:37:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217920_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 217920_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218061_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218061_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218063_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218063_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:25:45.49 +62:36:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218114_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218114_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:57:26.44 +64:12:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218155_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218155_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218161_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218161_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218167_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218167_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218188_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218188_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218287_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218287_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:07:56.77 +64:14:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218299_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218299_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:43:13.12 +65:18:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218428_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218428_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:04:51.89 +63:05:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218475_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218475_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:47:19.39 +60:43:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 218481_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218481_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218489_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218489_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218490_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218490_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218621_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218621_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218630_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218630_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:54:30.55 +60:49:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218652_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218652_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 218681_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218681_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:47:44.09 +63:52:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218738_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 218738_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219081_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219081_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:11:53.21 +60:43:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219105_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219105_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:03:43.99 +63:05:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.253 2205940115707385088 330.93129556196 +63.08334299270 13.3758 12.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219161_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219161_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219290_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219290_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:47:08.80 +60:40:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.207 2203629865675059328 326.78676125161 +60.67625062295 13.1354 12.2443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219399_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 219399_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 219404_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219404_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219406_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219406_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:23:07.35 +62:26:34.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 219413_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219413_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:02:43.67 +59:32:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219473_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219473_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:11:30.00 +61:35:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219573_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219573_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:01:36.58 +61:32:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219631_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219631_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219637_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219637_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219638_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219638_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219658_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219658_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219701_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219701_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:55:49.62 +62:17:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219881_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219881_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:26:56.28 +60:20:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.823 2191703604795700224 321.73433760914 +60.34261435689 13.4204 12.8844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219963_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219963_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 219994_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 219994_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:29:15.66 +58:22:47.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 220073_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220073_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:29:09.20 +60:40:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.841 2201340716827546624 337.28986382054 +60.67450924559 12.8666 11.7634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 220079_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220079_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220380_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220380_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220415_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220415_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220449_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220449_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220467_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220467_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220506_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220506_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220590_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220590_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220597_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220597_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:37:45.49 +59:26:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.258 2179639041658936704 324.44107691843 +59.44640279600 13.3501 12.4429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 220614_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220614_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:55:44.35 +62:19:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220792_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220792_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220814_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220814_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220815_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220815_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220877_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220877_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220884_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220884_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:03:28.28 +61:27:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 220915_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220915_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 220969_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 220969_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221080_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221080_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221083_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221083_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221169_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221169_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221248_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221248_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221370_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221370_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:44:44.03 +58:51:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.245 2202620587032741632 326.18280907581 +58.85716661516 13.8473 13.2568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 221509_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221509_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:03:17.62 +62:19:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221511_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221511_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:47:09.54 +64:10:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.491 2211314077564879616 341.79283092740 +64.16819632776 13.9706 13.1407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 221612_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221612_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:26:49.69 +63:44:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221673_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221673_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:05:06.12 +63:06:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221738_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221738_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221766_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221766_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 221847_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221847_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:26:13.58 +58:00:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221871_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 221871_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:24:08.43 +59:43:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221953_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 221953_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 222050_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222050_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222065_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222065_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:32:30.80 +65:18:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 222201_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222201_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222215_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 222215_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 222429_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 222429_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 222488_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222488_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:56:19.43 +63:42:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 222522_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222522_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222598_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222598_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222659_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222659_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222677_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222677_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222812_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222812_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:07:22.41 +62:01:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.814 2204889257472957440 331.84578306451 +62.03268812144 13.6941 12.7689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 222906_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222906_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 222930_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 222930_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223046_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223046_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223183_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223183_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:16:46.38 +63:42:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223229_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223229_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223290_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223290_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:54:34.02 +62:37:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223296_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223296_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223397_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 223397_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 223540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223553_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:52:42.77 +64:56:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.697 2217647475000240384 328.17883383710 +64.93922310356 13.8271 12.9513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 223609_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223609_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223794_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223794_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 223806_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223806_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:35:41.91 +64:39:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 223829_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224092_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224092_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224112_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224112_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224210_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 224210_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 224316_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224316_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224325_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224325_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224359_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224359_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224456_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224456_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224487_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224487_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224502_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224502_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224538_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224538_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224566_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224566_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224619_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224619_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224717_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224717_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224740_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224740_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224768_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224768_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224772_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224772_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224812_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224812_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224874_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224874_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 224968_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 224968_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225043_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225043_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225162_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225162_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225298_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225298_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225313_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225313_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225393_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225393_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225544_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225544_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225624_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225624_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225736_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225736_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225896_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225896_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225923_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225923_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 225954_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 225954_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226021_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226021_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226058_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226058_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226101_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226101_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226144_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226144_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226183_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226183_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226185_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226185_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226368_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226368_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226390_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226390_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226479_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226479_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226666_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226666_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226672_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226672_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226696_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226696_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226717_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226717_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226735_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 226735_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 226750_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226750_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226765_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226765_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226794_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226794_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 226830_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226830_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:30:25.56 +61:02:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.994 2192025521181925888 322.60677623047 +61.04629572901 14.3913 13.5128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 226893_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 226893_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227009_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227009_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227058_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227058_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227074_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227074_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227105_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227105_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227165_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227165_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227205_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227205_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227275_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227275_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227337_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227337_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:44:57.31 +58:34:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227377_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227377_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227402_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227402_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227408_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227408_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227437_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227437_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227439_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227439_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227497_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227497_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227596_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227596_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227633_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227633_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227635_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227635_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227643_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227643_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227663_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227663_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 227698_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 227698_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 151188_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 151188_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 212954_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 212954_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 16755_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 16755_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 77820_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 77820_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 44350_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 44350_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 49906_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 49906_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 119897_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 119897_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 21494_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 21494_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 71541_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 71541_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:50:07.96 +61:45:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.291 2207085768160649216 342.53483844962 +61.75765250920 12.1128 10.5071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 104540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 110070_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 110070_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 21:53:46.28 +60:32:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185589_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 185589_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 88064_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 88064_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 131838_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 131838_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:49:16.41 +58:35:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130686_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 130686_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117593_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 117593_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20676_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 20676_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 23:04:28.99 +64:45:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145832_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 145832_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 108270_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 108270_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:25:53.44 +60:20:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209799_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 209799_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 139700_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 139700_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:36:42.56 +57:44:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37150_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 37150_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:06:33.67 +64:39:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122543_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 122543_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 106663_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 106663_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:47:25.38 +59:57:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75972_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 75972_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 86226_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 86226_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:37:36.10 +61:16:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42578_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 42578_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73422_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 73422_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 99006_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 99006_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:50:24.93 +60:15:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145074_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 145074_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:26:40.33 +58:31:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 199540_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:49:46.49 +57:39:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 174880_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 174880_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 92206_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 92206_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 76639_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 76639_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
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Considering the candidate 133507_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 133507_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:40:59.59 +58:44:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83927_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
The candidate 83927_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423 did not pass the final checks
**** FOUND 22:14:48.62 +61:44:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198591_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
Preparing report for the candidate 198591_fd_Cep-06-Q2b1x1_2026-03-21_04-44-15_20.00sec_-14.90C_LIGHT_0423
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 41s
Prepared the HTML report for the field Cep-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:37:20.55 +60:18:47.8
22:34:54.66 +59:43:44.3
22:43:12.58 +59:21:53.5
22:11:22.54 +59:21:40.2
22:23:58.58 +58:50:00.1
23:14:41.26 +64:39:59.6
22:13:58.30 +57:48:10.9
23:07:30.25 +65:11:55.2
22:53:59.93 +63:47:43.2
21:46:52.07 +64:36:02.5
22:40:19.25 +60:12:09.9
21:48:36.99 +59:47:41.1
22:44:42.79 +65:11:27.0
21:46:56.19 +64:35:52.7
23:12:57.93 +64:24:50.3
21:44:48.54 +63:16:34.0
21:28:07.50 +61:16:34.7
22:08:36.89 +62:44:26.9
23:00:34.03 +63:16:23.0
22:04:50.28 +58:37:00.8
22:22:29.98 +64:09:19.3
22:30:42.45 +63:56:59.3
22:36:30.59 +63:25:52.1
22:41:46.35 +61:42:39.2
22:20:08.37 +62:10:11.8
22:54:20.40 +60:48:40.6
22:40:27.34 +60:53:43.6
########### Completed Cep-06-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 ####
22:53:59.93 +63:47:43.2
21:46:52.07 +64:36:02.5
22:40:19.25 +60:12:09.9
21:48:36.99 +59:47:41.1
21:46:56.19 +64:35:52.7
23:12:57.93 +64:24:50.3
21:44:48.54 +63:16:34.0
21:28:07.50 +61:16:34.7
22:08:36.89 +62:44:26.9
23:00:34.03 +63:16:23.0
22:04:50.28 +58:37:00.8
22:23:58.58 +58:50:00.1
23:14:41.26 +64:39:59.6
22:30:42.45 +63:56:59.3
22:36:30.59 +63:25:52.1
22:43:12.58 +59:21:53.5
22:44:42.79 +65:11:27.0
22:37:20.55 +60:18:47.8
22:54:20.40 +60:48:40.6
22:11:22.54 +59:21:40.2
22:34:54.66 +59:43:44.3
22:41:46.35 +61:42:39.2
22:22:29.98 +64:09:19.3
22:13:58.30 +57:48:10.9
22:40:27.34 +60:53:43.6
22:20:08.37 +62:10:11.8
23:07:30.25 +65:11:55.2
###################################################################################
22:53:59.93 +63:47:43.2 -- not an asteroid (will add it to exclusion list)
21:46:52.07 +64:36:02.5 -- not an asteroid (will add it to exclusion list)
22:40:19.25 +60:12:09.9 -- not an asteroid (will add it to exclusion list)
21:48:36.99 +59:47:41.1 -- not an asteroid (will add it to exclusion list)
21:46:56.19 +64:35:52.7 -- not an asteroid (will add it to exclusion list)
23:12:57.93 +64:24:50.3 -- not an asteroid (will add it to exclusion list)
21:44:48.54 +63:16:34.0 -- not an asteroid (will add it to exclusion list)
21:28:07.50 +61:16:34.7 -- not an asteroid (will add it to exclusion list)
22:08:36.89 +62:44:26.9 -- not an asteroid (will add it to exclusion list)
23:00:34.03 +63:16:23.0 -- not an asteroid (will add it to exclusion list)
22:04:50.28 +58:37:00.8 -- not an asteroid (will add it to exclusion list)
22:23:58.58 +58:50:00.1 -- not an asteroid (will add it to exclusion list)
23:14:41.26 +64:39:59.6 -- not an asteroid (will add it to exclusion list)
22:30:42.45 +63:56:59.3 -- not an asteroid (will add it to exclusion list)
22:36:30.59 +63:25:52.1 -- not an asteroid (will add it to exclusion list)
22:43:12.58 +59:21:53.5 -- not an asteroid (will add it to exclusion list)
22:44:42.79 +65:11:27.0 -- not an asteroid (will add it to exclusion list)
22:37:20.55 +60:18:47.8 -- not an asteroid (will add it to exclusion list)
22:54:20.40 +60:48:40.6 -- not an asteroid (will add it to exclusion list)
22:11:22.54 +59:21:40.2 -- not an asteroid (will add it to exclusion list)
22:34:54.66 +59:43:44.3 -- not an asteroid (will add it to exclusion list)
22:41:46.35 +61:42:39.2 -- not an asteroid (will add it to exclusion list)
22:22:29.98 +64:09:19.3 -- not an asteroid (will add it to exclusion list)
22:13:58.30 +57:48:10.9 -- not an asteroid (will add it to exclusion list)
22:40:27.34 +60:53:43.6 -- not an asteroid (will add it to exclusion list)
22:20:08.37 +62:10:11.8 -- not an asteroid (will add it to exclusion list)
23:07:30.25 +65:11:55.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:28:07.50 +61:16:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:48.54 +63:16:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:52.07 +64:36:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:56.19 +64:35:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:48:36.99 +59:47:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:50.28 +58:37:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:36.89 +62:44:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:22.54 +59:21:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:58.30 +57:48:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:08.37 +62:10:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:29.98 +64:09:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:58.58 +58:50:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:30:42.45 +63:56:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:34:54.66 +59:43:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:36:30.59 +63:25:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:37:20.55 +60:18:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:19.25 +60:12:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:27.34 +60:53:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:41:46.35 +61:42:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:43:12.58 +59:21:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:44:42.79 +65:11:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:53:59.93 +63:47:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:54:20.40 +60:48:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:00:34.03 +63:16:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:07:30.25 +65:11:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:57.93 +64:24:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:41.26 +64:39:59.6 -- 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)
21:28:07.50 +61:16:34.7 -- not a known variable star
21:44:48.54 +63:16:34.0 -- not a known variable star
21:46:52.07 +64:36:02.5 -- a known variable star
21:46:56.19 +64:35:52.7 -- not a known variable star
21:48:36.99 +59:47:41.1 -- a known variable star
22:04:50.28 +58:37:00.8 -- not a known variable star
22:08:36.89 +62:44:26.9 -- not a known variable star
22:11:22.54 +59:21:40.2 -- a known variable star
22:13:58.30 +57:48:10.9 -- a known variable star
22:20:08.37 +62:10:11.8 -- a known variable star
22:22:29.98 +64:09:19.3 -- a known variable star
22:23:58.58 +58:50:00.1 -- a known variable star
22:30:42.45 +63:56:59.3 -- a known variable star
22:34:54.66 +59:43:44.3 -- a known variable star
22:36:30.59 +63:25:52.1 -- a known variable star
22:37:20.55 +60:18:47.8 -- a known variable star
22:40:19.25 +60:12:09.9 -- a known variable star
22:40:27.34 +60:53:43.6 -- a known variable star
22:41:46.35 +61:42:39.2 -- a known variable star
22:43:12.58 +59:21:53.5 -- a known variable star
22:44:42.79 +65:11:27.0 -- a known variable star
22:53:59.93 +63:47:43.2 -- not a known variable star
22:54:20.40 +60:48:40.6 -- a known variable star
23:00:34.03 +63:16:23.0 -- a known variable star
23:07:30.25 +65:11:55.2 -- a known variable star
23:12:57.93 +64:24:50.3 -- a known variable star
23:14:41.26 +64:39:59.6 -- a known variable star
Found 6 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
27 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 ####
21:28:07.50 +61:16:34.7
21:44:48.54 +63:16:34.0
21:46:52.07 +64:36:02.5
21:46:56.19 +64:35:52.7
21:48:36.99 +59:47:41.1
22:04:50.28 +58:37:00.8
22:08:36.89 +62:44:26.9
22:11:22.54 +59:21:40.2
22:13:58.30 +57:48:10.9
22:20:08.37 +62:10:11.8
22:22:29.98 +64:09:19.3
22:23:58.58 +58:50:00.1
22:30:42.45 +63:56:59.3
22:34:54.66 +59:43:44.3
22:36:30.59 +63:25:52.1
22:37:20.55 +60:18:47.8
22:40:19.25 +60:12:09.9
22:40:27.34 +60:53:43.6
22:41:46.35 +61:42:39.2
22:43:12.58 +59:21:53.5
22:44:42.79 +65:11:27.0
22:53:59.93 +63:47:43.2
22:54:20.40 +60:48:40.6
23:00:34.03 +63:16:23.0
23:07:30.25 +65:11:55.2
23:12:57.93 +64:24:50.3
23:14:41.26 +64:39:59.6
22:34:54.71 +59:43:44.2
22:30:42.49 +63:56:59.3
22:31:57.02 +60:13:50.1
22:19:14.06 +61:22:37.5
22:15:34.25 +62:22:24.8
22:26:26.51 +63:06:40.5
22:55:39.43 +62:50:58.4
22:51:19.05 +65:01:08.5
22:49:46.49 +57:39:02.4
22:27:19.32 +64:45:48.2
21:48:31.30 +58:52:13.5
21:45:11.66 +61:08:29.7
22:03:55.78 +64:35:36.3
22:03:43.99 +63:05:00.0
21:47:08.80 +60:40:31.3
21:26:56.28 +60:20:29.6
22:29:09.20 +60:40:25.5
21:37:45.49 +59:26:45.4
21:44:44.03 +58:51:25.5
22:47:09.54 +64:10:02.9
22:07:22.41 +62:01:55.1
21:52:42.77 +64:56:19.8
21:30:25.56 +61:02:42.7
22:50:07.96 +61:45:25.9
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The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461120.90533404 -observatory 500
22:37:53.86 -07:44:04.2 Mercury (1.0mag)
01:08:25.25 +06:21:10.0 Venus (-3.9mag)
23:04:21.06 -07:06:53.9 Mars (1.2mag)
07:04:49.18 +22:57:56.7 Jupiter (-2.3mag)
00:17:32.06 -00:24:58.6 Saturn (0.9mag)
03:42:59.82 +19:32:04.9 Uranus (5.8mag)
00:07:20.78 -00:37:40.4 Neptune (7.8mag)
20:32:02.50 -22:53:44.4 Pluto (14.5mag)
01:51:26.73 +15:55:25.3 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Mar 21 04:46 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461120.90533404:
07:04:48.90 +22:57:54.0 Io (5.6mag)
07:04:37.23 +22:58:21.2 Europa (5.7mag)
07:04:27.21 +22:58:37.6 Ganymede (5.2mag)
07:04:12.10 +22:59:01.7 Callisto (6.4mag)
07:08:50.41 +22:59:19.3 Himalia (15.2mag)
07:04:49.61 +22:57:53.0 Thebe (16.0mag)
07:08:25.76 +23:22:46.9 Elara (17.2mag)
07:01:58.77 +23:51:24.7 Pasiphae (17.2mag)
07:13:36.29 +22:52:28.5 Carme (18.3mag)
00:17:27.54 -00:24:56.4 Titan (8.8mag)
00:17:37.82 -00:24:56.4 Rhea (10.1mag)
00:18:01.45 -00:22:55.1 Iapetus (11.5mag)
00:17:47.32 -00:25:02.8 Hyperion (14.8mag)
00:19:25.99 -00:13:44.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 21 04:46 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461120.90533404:
12:53:16.21 +08:25:27.5 JWST
16:58:20.97 +44:41:39.0 Chandra
08:52:36.46 -45:59:34.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 21 04:46 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461120.90533404 -observatory 500
18:35:45.19 -27:28:47.0 14.0mag P/2010 H2 (Vales)
04:51:21.11 -71:00:37.1 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:45.51 +31:17:59.5 17.0mag C/2017 K2 (PANSTARRS)
17:29:41.97 +07:27:13.4 17.6mag C/2021 G2 (ATLAS)
23:01:42.99 +28:26:38.1 16.9mag C/2022 E2 (ATLAS)
04:00:54.87 +25:18:21.7 15.7mag C/2022 N2 (PANSTARRS)
09:01:50.94 +31:27:53.7 16.0mag C/2022 QE78 (ATLAS)
08:30:09.46 -03:07:35.5 17.2mag C/2022 R6 (PANSTARRS)
18:56:30.24 +16:19:35.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:19.00 -11:50:31.0 17.6mag P/2023 B1 (PANSTARRS)
09:24:11.47 -16:15:22.8 17.4mag C/2023 F3 (ATLAS)
21:22:18.10 +61:42:37.4 17.4mag C/2023 H5 (Lemmon)
19:33:05.74 -03:31:18.2 14.5mag C/2023 R1 (PANSTARRS)
21:36:42.06 +82:53:32.4 17.7mag C/2023 X2 (Lemmon)
06:15:16.08 +63:46:50.4 16.8mag C/2024 A1 (ATLAS)
04:07:42.65 +05:30:14.5 9.1mag C/2024 E1 (Wierzchos)
11:22:18.20 +02:48:39.3 18.0mag C/2024 G2 (ATLAS)
16:32:08.10 +02:13:41.9 17.5mag C/2024 G6 (ATLAS)
20:10:16.28 +08:51:24.8 14.9mag C/2024 J3 (ATLAS)
03:05:00.65 -26:34:57.6 16.5mag C/2024 T5 (ATLAS)
04:57:46.70 +52:28:37.6 17.6mag C/2025 J1 (Borisov)
15:12:40.89 +18:00:48.7 14.4mag C/2025 L1 (ATLAS)
02:49:01.90 -22:37:50.3 17.6mag C/2025 Q3 (ATLAS)
22:33:10.30 +19:02:35.7 12.4mag C/2025 R3 (PANSTARRS)
13:04:54.81 +01:20:20.4 17.6mag C/2025 Y1 (ATLAS)
02:08:47.27 -06:07:04.9 14.0mag C/2026 A1 (MAPS)
22:40:16.54 +31:09:56.9 13.7mag C/2026 B2 (Sun-Gao)
17:52:51.61 -10:49:46.8 13.3mag 10P/Tempel
15:26:35.22 +05:06:58.2 11.8mag 24P/Schaumasse
11:11:49.65 -02:27:55.6 15.6mag 29P/Schwassmann-Wachmann
17:44:04.66 -10:37:48.8 17.3mag 40P/Vaisala
10:44:56.37 -06:31:29.1 16.4mag 43P/Wolf-Harrington
01:09:34.08 +12:59:46.1 17.0mag 47P/Ashbrook-Jackson
06:29:08.09 +42:16:07.8 17.1mag 63P/Wild
22:54:45.99 -14:41:20.9 15.7mag 65P/Gunn
02:59:24.08 +11:29:27.7 15.9mag 76P/West-Kohoutek-Ikemura
00:10:21.93 +03:07:45.7 14.6mag 78P/Gehrels
21:40:08.46 -16:38:21.1 14.5mag 88P/Howell
01:01:47.08 +13:20:50.7 15.2mag 93P/Lovas
04:11:12.50 +30:42:44.5 16.5mag 123P/West-Hartley
08:07:54.35 +50:05:06.4 16.2mag 124P/Mrkos
01:54:55.25 +11:24:08.9 16.4mag 128P/Shoemaker-Holt
01:58:09.98 +11:05:27.0 17.4mag 131P/Mueller
23:21:52.23 +03:15:37.8 12.9mag 141P/Machholz
23:31:59.75 -04:18:10.0 13.0mag 141P-A/Machholz
22:32:29.31 -06:52:31.0 16.0mag 141P-D/Machholz
23:51:31.46 -13:57:44.3 15.5mag 162P/SidingSpring
10:39:04.34 +32:01:59.5 17.5mag 164P/Christensen
05:50:25.49 +24:44:09.6 17.5mag 198P/ODAS
15:32:49.80 -03:19:06.0 16.9mag 210P/Christensen
20:13:22.27 -17:27:41.5 17.2mag 218P/LINEAR
16:59:41.95 -16:38:29.1 16.3mag 235P/LINEAR
04:42:12.72 +32:03:11.1 16.3mag 240P/NEAT
07:29:56.71 -08:19:06.6 17.5mag 242P/Spahr
15:48:33.27 +05:08:03.1 17.7mag 391P/Kowalski
07:28:01.66 +21:06:51.2 17.5mag 450P/LONEOS
05:01:26.80 +46:35:27.7 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 21 04:46 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
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
-rw-r--r-- 1 apache apache 5.7K Mar 21 04:46 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 21 04:46 tocp_transients_list.txt