This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857
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!
TCP 2026 03 27.0902* 01 09 49.90 +65 08 28.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0109489+650828,2461126.5902,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0109489+650828 20260327.0902 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:09:49.90 +65:08:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.0902 2461126.5902 12.95 00:58:58.47 +59:04:51.6
123.90202 -3.77655 galactic Cas Second-epoch detections are separated by 4.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J014.7383+59.0860 | 00:58:58.47 +59:04:51.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 00 58 58.47 +59 04 51.6 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.7383+59.0860,2461126.5902,12.95,0.05,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 J014.7383+59.0860 20260327.0902 12.95CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:58:58.47 +59:04:51.6 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 01 39 56.81 +60 52 21.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013956.73+605213.0,2461126.5902,13.24,0.05,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 J013956.73+605213.0 20260327.0902 13.24CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:56.81 +60:52:21.1 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.0902 2461126.5902 13.40 02:42:54.77 +63:23:40.4
135.03464 3.17300 galactic Cas Second-epoch detections are separated by 2.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:42:54.77 +63:23:40.4 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 02 42 54.77 +63 23 40.4 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.5902,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.0902 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:42:54.77 +63:23:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 00 57 36.46 +61 28 10.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1675692,2461126.5902,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1675692 20260327.0902 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:36.46 +61:28:10.8 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 01 27 44.54 +62 06 42.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1696374,2461126.5902,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1696374 20260327.0902 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:27:44.54 +62:06:42.5 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 02 20 32.51 +62 32 02.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0933 Cas,2461126.5902,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0933 Cas 20260327.0902 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:20:32.51 +62:32:02.6 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 01 12 11.44 +59 57 30.5 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0112111+595728,2461126.5902,12.41,0.05,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
NSVS J0112111+595728 20260327.0902 12.41CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:12:11.44 +59:57:30.5 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 01 47 55.67 +64 32 55.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0147560+643254,2461126.5902,12.63,0.05,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 J0147560+643254 20260327.0902 12.63CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:55.67 +64:32:55.9 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 02 16 49.17 +63 45 56.7 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0216499+634557,2461126.5902,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0216499+634557 20260327.0902 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:16:49.17 +63:45:56.7 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.0902 2461126.5902 9.80 00:58:48.49 +58:03:57.9
123.90982 -4.79167 galactic Cas Second-epoch detections are separated by 1.4" and 6.5 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 J014.7051+58.0558 | 00:58:48.52 +58:03:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 00 58 48.49 +58 03 57.9 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.7051+58.0558,2461126.5902,9.80,0.05,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
ATO J014.7051+58.0558 20260327.0902 9.80CV 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/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:58:48.49 +58:03:57.9 ;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_Cas-03-Q2b1x1_2026-01-08_19-54-29_20_00sec_-14_90C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20_00sec_-14_90C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20_00sec_-14_90C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20_00sec_-14_90C_LIGHT_0017_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.0902* 01 08 40.76 +61 16 12.4 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 407,2461126.5902,12.15,0.05,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
NSV 407 20260327.0902 12.15CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:08:40.76 +61:16:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.57895757 09.01.2026 01:53:31.934 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461049.57895757 09.01.2026 01:53:31.934 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.59088545 27.03.2026 02:10:42.503 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
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: 10 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): 23878
Objects passed selection criteria: 23772
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 18450.2
Average stars matched: 17912 (97.0827 %)
Memory usage VmPeak: 129296 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 21:13:00 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: 2461049.57895757 09.01.2026 01:53:31.934 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
First image: 2461049.57895757 09.01.2026 01:53:31.934 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Last image: 2461126.59088545 27.03.2026 02:10:42.503 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 143
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 199 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): 182788
Objects passed selection criteria: 182273
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 138468
Average stars matched: 133239 (96.2235 %)
Memory usage VmPeak: 2406748 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 21:19:45 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.58956189
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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits'
wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits'
wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits'
wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:59.457 +61:58:39.69
Second-epoch image center 01:42:35.786 +62:00:57.55
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:59.457 +61:58:39.69
Second-epoch image center 01:42:33.412 +62:00:27.10
Angular distance between the image centers 0.06 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 01:42:35.786 +62:00:57.55
Second-epoch second image center 01:42:33.412 +62:00:27.10
Angular distance between the image centers 0.00965 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.EVcbNhFVhW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits &> /tmp/tmp.D1Y5hAbm7v
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits &> /tmp/tmp.Mp3OeV3jvD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits &> /tmp/tmp.MgNweZFpsa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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 16167 out of 30070 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.965914
a=0.000000 b=1.000000 c=22.965914
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
2.1 pix Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
2.8 pix fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
14.1 mag. fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
14.2 mag. fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EVcbNhFVhW (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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3738, passed=30070
Got 30070 stars (including 26294 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 30070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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: 0.46"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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.D1Y5hAbm7v (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/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=12, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3698, passed=29938
Got 29938 stars (including 26206 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 29938 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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: 0.39"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits -region wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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.Mp3OeV3jvD (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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=993, passed=12827
Got 12827 stars (including 11827 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 12827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 977 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 973 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MgNweZFpsa (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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1079, passed=13331
Got 13331 stars (including 12245 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 13331 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out03608.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51881_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 51881_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:38:01.02 +63:01:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13807_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 13807_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:25:02.47 +61:04:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07129_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 07129_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:30:27.26 +62:31:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03608_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 03608_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:09:49.90 +65:08:28.4
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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:59.457 +61:58:39.69
Second-epoch image center 01:42:35.786 +62:00:57.55
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:59.457 +61:58:39.69
Second-epoch image center 01:42:33.412 +62:00:27.10
Angular distance between the image centers 0.06 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 01:42:35.786 +62:00:57.55
Second-epoch second image center 01:42:33.412 +62:00:27.10
Angular distance between the image centers 0.00965 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits &> /tmp/tmp.QRC3VKBly8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits &> /tmp/tmp.GLhYIz4bqU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits &> /tmp/tmp.ZxOAYlMF3z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits &> /tmp/tmp.8ZotoNGkJg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits and wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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 16766 out of 227084 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.818320
a=0.000000 b=1.000000 c=22.818320
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 103 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
1.9 pix Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
2.7 pix fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Limiting magnitude estimates:
15.5 mag. Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
15.5 mag. Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
14.1 mag. fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
14.3 mag. fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QRC3VKBly8 (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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=35652, passed=227031
Got 227031 stars (including 191032 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 227031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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: 0.46"
Estimated accuracy of the plate solution: 0.43"
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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits -region wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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.GLhYIz4bqU (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/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=35473, passed=226301
Got 226301 stars (including 190511 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 226301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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: 0.43"
Estimated accuracy of the plate solution: 0.43"
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_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits -region wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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.ZxOAYlMF3z (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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=7724, passed=77892
Got 77892 stars (including 70098 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 77892 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 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: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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: 0.69"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8ZotoNGkJg (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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=7970, passed=91886
Got 91886 stars (including 83821 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 91886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 968 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.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_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-08-48_20.00sec_-10.00C_LIGHT_0010.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-03-Q2b1x1_211118_TTUQ2b1x1_7374_LWYQ6857/wcs_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out157328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out239349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97114.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 255374_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255374_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:18:27.83 +59:13:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.977 459190522882200064 034.61621947678 +59.22120810029 13.7720 13.2030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255375_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255375_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:52:46.68 +64:21:16.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 255377_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255377_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:32:48.18 +64:28:34.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 255381_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255381_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:53:55.32 +58:29:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.272 506208659437533440 028.48055934079 +58.48459247558 13.0324 12.0248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255383_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255383_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:43:26.35 +63:20:05.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 255386_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255386_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:27:17.58 +58:06:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.069 458861562746337536 036.82472243950 +58.10576246329 14.2412 13.7101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255387_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255387_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:32:22.39 +60:27:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.065 509836330565344768 023.09242308918 +60.45864559454 13.4073 12.8057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255390_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 255390_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 255392_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255392_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:43:01.78 +63:22:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.370 512080914828741632 025.75743466864 +63.36806391516 12.4311 10.9992 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255400_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255400_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 255401_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255401_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:40:00.30 +60:52:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.315 509927590028710784 025.00199794115 +60.88202963679 13.0308 11.9564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255402_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255402_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:56:38.29 +58:14:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.770 424385825901591424 014.16066202162 +58.24789445808 12.1159 11.5311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255406_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255406_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:51:54.17 +64:45:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.651 518225432478541568 027.97573443928 +64.75951399079 12.5355 11.5909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255408_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255408_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:03:21.43 +57:48:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255869_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255869_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:38:00.46 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255970_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 255970_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:19:12.35 +65:36:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256038_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256038_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:17:59.11 +57:47:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256052_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256052_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 256056_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256056_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:58:16.31 +59:38:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.566 507862844627662720 029.56967079484 +59.65034352526 12.8236 12.4000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256161_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256161_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:33:42.04 +58:17:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.541 509005443366790272 023.42590234846 +58.29356661966 12.4863 12.0694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256164_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256164_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:03:46.64 +61:03:22.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256175_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256175_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:53:16.34 +61:08:55.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256178_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256178_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:05:03.63 +64:21:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.901 515060075945586176 031.26502482935 +64.36397361378 12.6511 11.9459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256222_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256222_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:46:34.59 +61:10:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.468 511216969261895936 026.64580891928 +61.17719999203 12.9610 12.3726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256280_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256280_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:37:00.50 +59:37:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256292_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256292_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:00:51.84 +58:31:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.199 505508446637646592 030.21645161399 +58.52382030882 12.9664 12.6563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256332_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256332_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:23:23.53 +63:36:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.840 514342575887502464 035.84909384475 +63.60387735364 12.5425 11.4782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256362_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256362_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:15:58.96 +63:12:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256378_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256378_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:27:49.80 +62:54:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.915 514075532000750720 036.95804085135 +62.91256327280 13.0065 12.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256388_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256388_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:13:29.99 +58:34:25.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256389_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256389_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:38:45.65 +62:35:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256391_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256391_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:43:53.40 +61:53:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256393_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256393_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:02:54.72 +64:24:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256398_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256398_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:53:03.27 +60:35:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256416_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256416_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:46:33.64 +61:16:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.518 511219378749345152 026.64035262574 +61.27991602603 12.8700 12.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256417_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256417_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:38:33.18 +60:48:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.303 509905634154578560 024.63764517723 +60.80015133430 13.1380 12.7581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256429_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256429_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:03:36.63 +61:03:02.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256439_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256439_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:04:32.42 +57:59:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256440_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256440_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:51:02.79 +64:49:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.376 518229590006827648 027.75942395447 +64.83128019779 12.9799 12.3873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256442_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256442_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:16:08.17 +58:49:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256454_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256454_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:43:03.36 +58:08:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256487_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256487_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:20:18.26 +58:13:43.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256493_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256493_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:30:09.00 +57:48:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256509_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256509_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:08:25.20 +58:25:23.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256521_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256521_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:20:11.00 +58:12:09.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256594_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256594_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:22:13.23 +59:08:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.028 459200143609929216 035.55628920754 +59.13954670009 13.7928 13.2385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256663_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256663_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:00:36.74 +58:30:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256673_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256673_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:04:27.10 +65:05:55.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256676_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256676_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:14:29.82 +63:16:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256691_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256691_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:17:21.70 +59:22:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.809 507234508089993472 034.34003720349 +59.37580184164 13.3423 12.7680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256697_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256697_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:00:36.25 +63:32:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.956 523357845376882304 015.15346734270 +63.54609147647 12.3183 11.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256698_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256698_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:01:15.09 +59:23:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.038 507816562059228544 030.31354850954 +59.38368853525 13.3052 12.6838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256706_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256706_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:19:57.74 +59:32:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.769 459224057987492224 034.99153878575 +59.54094426487 13.2778 12.7155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256712_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256712_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:33:22.99 +57:44:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256727_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256727_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:19:03.85 +63:57:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256729_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256729_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:38:08.10 +61:03:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.911 509945800689898496 024.53645990448 +61.06601549831 13.5746 13.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256746_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256746_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:58:40.01 +59:16:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.752 507801031456497792 029.66851337035 +59.26623741797 13.3412 12.6434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256787_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256787_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:08:30.46 +58:24:18.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256824_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 256824_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 256826_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256826_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:01:36.80 +59:57:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.675 507939947877705600 030.40447218811 +59.95610706443 13.3816 12.7797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256827_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256827_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:44:56.54 +59:46:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256835_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256835_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:29:30.53 +60:40:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.662 465392730532552064 037.37615949945 +60.67792767616 13.5153 12.8403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256847_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256847_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:48:38.20 +61:49:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.351 511332143104791040 027.15857782551 +61.81904598779 12.7859 11.6380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256848_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256848_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:35:21.87 +61:07:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256866_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256866_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:46:13.86 +61:13:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.418 511264252570065024 026.55843669700 +61.22884126972 12.9862 12.3840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256886_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256886_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:20:14.46 +59:20:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.015 459212959792100480 035.06108979178 +59.33650085724 13.3437 12.7016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256915_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256915_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:24:58.08 +59:22:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.894 510049429657560576 021.24357840772 +59.38266033805 13.4525 12.7576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256928_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256928_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:35:54.52 +60:13:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.889 509780392908244224 023.97563084557 +60.22213797866 13.4292 12.9491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256937_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256937_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:41:51.62 +59:58:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.409 509586260387937024 025.46531647308 +59.97407088424 12.7494 11.6192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256939_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256939_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:21:29.00 +63:55:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.531 515135907886837888 035.37107965967 +63.92604441472 13.6113 12.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256961_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256961_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:23:30.27 +61:45:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.507 513545223794465152 035.87557546433 +61.75879839840 13.8041 13.0689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256973_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256973_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:10:32.24 +59:59:54.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 256977_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 256977_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:37:44.74 +64:45:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.497 513064183156209536 024.43624931833 +64.76456259326 13.3761 12.7197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257007_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257007_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:47:19.04 +63:38:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.969 512068064285526784 026.83066913927 +63.63662862749 13.4108 12.6889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257041_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257041_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:46:51.10 +60:39:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.192 511164678045195008 026.71100154417 +60.65281066062 13.6732 13.1253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257044_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257044_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:10:31.35 +60:57:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.385 507622326456919040 032.63010829315 +60.95120822338 13.6110 13.0028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257058_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257058_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:04:58.69 +64:24:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.071 515061312896144384 031.24417125294 +64.40841594645 13.2404 12.2759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257102_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257102_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:23:54.78 +66:08:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257103_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257103_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:14:00.46 +61:42:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257139_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 257139_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:38:06.50 +58:10:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.381 508962734211151616 024.52801987986 +58.17819905071 13.3107 12.3219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34587_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 34587_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 239124_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 239124_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:47:52.30 +61:11:15.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 63463_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 63463_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:30:27.25 +62:31:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64973_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 64973_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:14:53.90 +63:36:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46060_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 46060_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:38:00.96 +63:01:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109275_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 109275_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 97114_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 97114_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 70238_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 70238_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 159991_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 159991_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:58:32.64 +59:25:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.833 426041037577758592 014.63441178889 +59.41697340459 12.8666 11.9847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148123_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 148123_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 29256_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 29256_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 157328_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 157328_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:59:00.42 +59:32:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.812 426053574582188672 014.74915385953 +59.53423194781 12.2775 11.1536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187623_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 187623_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:59:07.59 +58:16:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39511_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 39511_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 16228_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 16228_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:05:28.22 +65:58:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44494_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 44494_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 72902_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 72902_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 01:45:35.77 +63:07:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173403_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 173403_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:56:42.75 +58:52:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239349_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 239349_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 239225_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 239225_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 00:59:43.71 +58:21:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.307 425692281929173504 014.92984602041 +58.36036980012 12.5225 11.7028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110267_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 110267_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks
**** FOUND 02:01:09.67 +61:03:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115274_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
Preparing report for the candidate 115274_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
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Considering the candidate 121833_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011
The candidate 121833_fd_Cas-03-Q2b1x1_2026-03-26_21-10-42_20.00sec_-10.00C_LIGHT_0011 did not pass the final checks